The galaxy presents as a centrally concentrated object with a smooth overall morphology, displaying a relatively round appearance. The light profile is generally smooth, showing a bulge-dominated structure with a gradual falloff in surface brightness from the core. There is little evidence of spiral arm structures or prominent dust lanes. The color gradient across the galaxy suggests a possible radial variation in stellar populations, with the central region appearing more yellow. This could indicate a higher concentration of older, redder stars in the nucleus compared to the outer regions, which seem slightly bluer. There are no obvious signs of significant ongoing major mergers or tidal disturbances.
