The galaxy presents as a centrally concentrated object with a generally smooth morphology. The light profile appears to be relatively featureless, lacking prominent spiral arms or a distinct bar structure. The core region exhibits a yellowish hue, suggesting a population of older stars, potentially indicating a lower rate of ongoing star formation in the central bulge. Moving outward from the center, a subtle transition to a bluer color is observed, which could suggest the presence of younger stellar populations in the outer regions, but the contribution of the older stars is considerable. The galaxy appears to have a slightly elliptical shape. No signs of major mergers or tidal disturbances are readily apparent in the image. Overall, the galaxy seems to be a relatively massive system with a predominantly smooth morphology.
