The galaxy presents as a relatively smooth, lenticular-like structure with a somewhat elliptical morphology. The core region exhibits a bright, concentrated luminosity, indicative of a high stellar density and/or active galactic nucleus presence.  There is an overall dominance of redder hues in its spectral output, suggesting an older stellar population and a diminished rate of star formation.  There appears to be a slight irregularity in the galactic profile, possibly hinting at minor gravitational interactions or a past merger event.  The overall light profile suggests a system transitioning toward a more passive, quiescent state.
