The galaxy presents as a single, concentrated luminous object. The light distribution appears relatively smooth, with a centrally concentrated bulge that dominates the galaxy's overall structure. There is a subtle color gradient visible, with the central region exhibiting a slightly yellower hue, possibly indicative of an older stellar population or higher dust content. The outer regions display a bluer tinge, which may point to the presence of younger stars. The galaxy exhibits a round morphology, lacking any obvious spiral arm features or a distinct disk component. No significant signs of tidal disruption, major mergers, or active galactic nuclei are observable. The overall structure suggests that this could be an elliptical galaxy, potentially with a lenticular (S0) morphology.
