The galaxy presents a generally elliptical morphology, with a smooth appearance dominating its overall structure. A slight elongation is observable, deviating marginally from a perfectly circular form. The central region exhibits a bright, concentrated luminosity, suggestive of a substantial stellar population and/or active galactic nucleus activity. Moving outwards from the core, the intensity of the light gradually diminishes, transitioning into a less defined halo. A subtle disc-like structure seems embedded within the body of the galaxy, with a slight angle of inclination relative to our line of sight. There are indications of internal dynamics or gravitational disturbances, manifesting as subtle irregularities in the light distribution, which could imply that a small minor merging event is in progress. The galaxy displays a color profile that indicates its stellar populations are largely composed of older, redder stars, with some regions showing slightly bluer hues, possibly suggestive of ongoing or recent star formation.
