The galaxy presents an elliptical morphology, though not perfectly spherical, suggesting a possible slight disk component or ongoing interaction. The central bulge is prominent and exhibits a yellowish hue, indicative of an older stellar population dominated by red giant stars. Moving outwards from the core, the galaxy displays a gradual fading and a subtle shift towards bluer colors in the outer regions, hinting at the presence of younger, hotter stars involved in some star formation, albeit at a low rate.

No significant tidal tails or strong distortions are visible, but a slight asymmetry in the outer regions is observed on one side of the galaxy, suggesting a possible past minor merger or disturbance. Overall, the galaxy appears relatively evolved, with a significant fraction of its stellar population being older, but with hints of recent or ongoing star formation activity.
