The galaxy exhibits a generally smooth morphology, with a slight elongation suggesting an elliptical or lenticular classification. It displays a concentrated central bulge, characterized by a yellow-orange hue indicative of an older stellar population. Fainter, diffuse blue regions can be observed at the edges of the galaxy, possibly indicating the presence of younger, hotter stars and ongoing star formation activity. There appears to be a minor disturbance or asymmetry in the galaxy's shape, potentially resulting from a past or ongoing interaction with a smaller galaxy, although no distinct tidal features or merging companions are readily apparent in the image.
