The observed galaxy presents as a disk galaxy, seen nearly edge-on from our vantage point. A prominent central bulge dominates the galaxy's luminosity, appearing smooth and spheroidal in shape. The bulge exhibits a yellowish-white color, potentially indicating an older stellar population. A disk is visible, extending outwards from the bulge. The disk appears relatively thin and is characterized by a bluer, more diffuse light, suggesting the presence of younger stars and potentially some ongoing star formation, although the rate is likely relatively low. There is no clear evidence of spiral arm structure in this image. There are no major tidal disturbances or indications of recent merger activity apparent in the galaxy's structure. The outer regions of the disk fade gradually into the background sky, making a precise determination of the galaxy's overall size difficult. The smooth appearance of the bulge suggests that it is likely the dominant mass component.
