The galaxy presents as a centrally concentrated, smooth, and relatively round object. There is a dominant, luminous core that fades gradually into the outer regions, indicating a lack of distinct structural features such as spiral arms or a bar. The color profile is broadly consistent across the galaxy, with a slight shift towards redder hues in the core as compared to the outer regions. There are no signs of significant tidal disturbances or ongoing major mergers. The overall morphology suggests the galaxy is likely an elliptical or S0 type. Based on the redder colors, this could indicate a population of older stars. The size of the galaxy suggests it is a moderately sized galaxy.
