The galaxy presents as a relatively smooth, elliptical form, elongated along a major axis. The central region exhibits a bright, concentrated core, suggestive of a significant stellar population and potentially an active galactic nucleus. Moving outward from the core, the luminosity gradually decreases, indicating a diminishing density of stars. The overall color appears consistent, trending towards a redder hue, which may signify an older stellar population with reduced ongoing star formation. Subtle irregularities are observed in the outer regions which might be evidence of tidal interactions with a small companion galaxy.
