The observed galaxy presents as a disk galaxy, viewed nearly edge-on from our vantage point. The galactic disk exhibits a clear asymmetry, with a brighter, slightly broader region towards what appears to be the central bulge, tapering off into a fainter and thinner disk. This suggests a possibly warped or otherwise disturbed morphology. The central bulge is characterized by a yellowish hue, indicative of an older stellar population and minimal ongoing star formation in that region. The disk itself shows a bluer tint, particularly at the edges and extending outwards, suggesting the presence of younger stars and recent or ongoing star formation. Faint dust lanes appear to be obscuring some of the light from the disk, particularly along the plane of the galaxy. There are potentially signs of tidal disturbances, such as subtle distortions or asymmetries in the disk shape. The galaxy is moderately sized with indications of relatively moderate star formation activity. The morphology seems more feature dominated than smooth. There is a potential merger happening with a portion of the disk being more disturbed than the rest of the galaxy. 
