The galaxy presents a relatively smooth and rounded morphology. It appears primarily elliptical in shape. The galaxy exhibits a centrally concentrated luminosity profile, with brightness decreasing smoothly from the core outwards. There is no obvious presence of spiral arms or a prominent disk structure. The color appears fairly uniform across the galaxy, suggesting an older stellar population and limited ongoing star formation. There is no evidence of significant tidal disturbances or interactions with other galaxies in its immediate vicinity. The galaxy does not exhibit any prominent dust lanes or distinct substructures within its main body. The overall color is somewhat redder than average, consistent with a galaxy dominated by older stars and a lower rate of star formation.
