The galaxy presents as a centrally concentrated, relatively smooth structure. The core is a bright, unresolved central bulge, exhibiting a luminosity gradient suggestive of a high stellar density. This bright central region is surrounded by a more diffuse halo or disk component. There is a subtle color gradient observed with the core appearing more blue-white, and the outer regions trending towards redder hues, possibly indicating an older stellar population or higher dust content in the outer disk. There is a lack of discernible spiral arm structure, though this could be a consequence of the viewing angle. The overall morphology suggests an early-type galaxy, likely an elliptical or lenticular galaxy, with a slight possibility of being a face on spiral with faint arms. There appear to be very little ongoing disturbances or mergers.
