The galaxy presents a generally smooth morphology, with no apparent spiral arms or a distinct bar structure. It is primarily elliptical in shape, exhibiting a moderate degree of ellipticity. The galaxy's light profile appears centrally concentrated with a gradual decrease in brightness towards the outer edges. It exhibits a color gradient, appearing bluer in the central regions and becoming redder outwards. There are no signs of active galactic nuclei (AGN) or intense star formation regions. There is no major disturbance to the overall form of the galaxy, such as from a possible merger. The light distribution does not exhibit any distinct shells or tidal features, and the overall structure suggest a relatively evolved system with little ongoing star formation.
