The galaxy presents an elongated, elliptical morphology. A bright, concentrated central bulge dominates the luminosity profile. The color gradient suggests a population of older stars in the bulge, appearing more yellow. Fainter, bluer light extends outwards from the central region, tracing a disk-like structure, though features are poorly resolved. The light from the disk fades significantly towards the edges. There are hints of possible dust lanes within the disk. Overall, the galaxy appears relatively smooth, with no strong evidence of ongoing major mergers, though faint structures suggest possible minor interactions or internal disturbances. The major axis of the galaxy is oriented diagonally in the image.
