The galaxy presents as a centrally concentrated object, exhibiting a roughly elliptical morphology. The core region displays a brighter, more intense luminosity, suggesting a high density of stars or possibly an active galactic nucleus. Moving outwards from the center, the galaxy gradually fades into a diffuse halo, indicating a decreasing stellar density. The galaxy's overall color appears moderately red, potentially indicative of an older stellar population or significant dust obscuration. Subtle hints of bluer regions are present, possibly indicating areas of more recent star formation, though these features are not prominently defined. There is no strong evidence of distinct spiral arms or a pronounced disk structure; the galaxy seems primarily spheroidal in nature, with a smooth overall appearance. Minor asymmetry is observed in the outer regions. It shows no signs of significant tidal disturbances or interaction with other galaxies.
