The galaxy presents a generally smooth and elliptical morphology. A bright, concentrated central bulge dominates the structure, exhibiting a yellowish-white hue, indicative of an older stellar population. Fainter, bluer light extends outwards from the bulge, forming a more diffuse halo. There is no clear evidence of spiral arms or a well-defined disk. The galaxy's overall shape is roughly in between round and elliptical. There are no obvious signs of ongoing major mergers or strong tidal disturbances; any disturbances appear minor. Given the color profile and morphology, this is likely an early-type galaxy, possibly an elliptical or lenticular. It is a relatively massive galaxy with an apparently low star formation rate.
