The galaxy presents as a single, concentrated light source. Its overall morphology is smooth and elliptical in appearance, showing a high degree of radial symmetry. There is a prominent central bulge, which appears to dominate the overall light profile. The light tapers off gradually from the core, displaying no discernable spiral arm structures or prominent disk features. The color index suggests a population of older stars, with a yellowish-red hue. Overall, the galaxy is likely an elliptical galaxy with little ongoing star formation. There is no visual evidence of any major tidal disturbances or ongoing mergers, although there are slight indications of possible tidal tails.
