The galaxy appears to be a luminous, relatively smooth object. Its morphology suggests a fairly elliptical shape. It exhibits a concentrated central bulge with a gradual decrease in luminosity towards its outer regions. The color profile appears to be generally redder, indicating a population of older stars and potentially a lower ongoing star formation rate. There is no clear evidence of significant spiral arm structure or major mergers. Subtle disturbances are difficult to rule out. The galaxy is observed to be quite massive.
