The galaxy appears as a centrally concentrated, largely featureless object with an overall elliptical morphology. The core is bright and unresolved, indicating a high stellar density in the galactic nucleus. There is evidence of some color variation. The central region has a slightly bluish hue, which might be from the presence of younger stars or a weak active galactic nucleus. The outer regions appear reddish, possibly indicative of an older stellar population or dust extinction. Overall, the galaxy seems to be relatively isolated with no clear signs of tidal interactions or major disturbances, although a slight asymmetry could point to a minor gravitational interaction. It is compact, consistent with a moderate-sized galaxy, and has an estimated distance of about 1.61 kpc based on the redshift information.
