The galaxy presents as a moderately luminous, disk-shaped structure with an overall smooth appearance. The central bulge exhibits a bright, concentrated luminosity, suggesting a significant population of older stars. The disk component displays a slightly elongated morphology. There is evidence of some disrupted features, such as an area on one side that appears to be somewhat disrupted with a different color, perhaps suggesting a minor interaction or internal disturbance. Overall, the galaxy appears to be in a late stage of its evolution, with low star formation activity. The overall light profile indicates that this galaxy is somewhere in between a pure elliptical and a spiral galaxy.
