The galaxy presents as a roughly elliptical, smooth, and relatively symmetrical structure. It exhibits a concentrated central bulge, appearing significantly brighter and more densely packed than its outer regions. The color profile suggests an older stellar population, characterized by a yellowish-red hue, particularly concentrated in the core. There is some evidence of bluer colors within the disk, indicating the presence of a younger stellar population. The galaxy shows no clear spiral arm structure or prominent dust lanes. It does not appear to be undergoing any major merger activity, though there is potentially some minor disturbance in its morphology. Overall, the galaxy appears to be a mature system with a substantial bulge component.
