The observed galaxy exhibits a primarily smooth morphology, suggesting an elliptical or lenticular classification. Its shape appears to be somewhere between round and elliptical but leaning towards elliptical. There may be evidence of minor disturbances within the galaxy's structure, such as faint tidal features. The galaxy presents a subtle color gradient, with a possibly redder hue at the core transitioning to slightly bluer hues in the outer regions. This could be suggestive of older stellar populations dominating the center and younger, hotter stars populating the outskirts. The galaxy appears as a centrally concentrated object with a diffuse halo. The relative lack of distinct features, such as spiral arms or prominent dust lanes, further supports the notion of a more evolved system. There does not appear to be a major ongoing merger.
