The galaxy presents a centrally concentrated morphology with a relatively smooth appearance. There's a bright, compact core that dominates the luminosity profile. The color of the core is a bright white, suggestive of a high stellar density and potentially ongoing star formation, or possibly an active galactic nucleus. Surrounding the core is a more diffuse halo-like structure, with a bluer hue. This suggests the presence of a younger stellar population in the outer regions, perhaps indicating recent or ongoing star formation. Subtle, slightly irregular features are present in the outer regions, hinting at possible tidal interactions or minor disturbances. While the overall structure is smooth, the presence of these irregularities could point to a past or ongoing minor merger event. The apparent size of the galaxy is relatively compact; its light is concentrated in a small angular extent. 
