The galaxy appears as a centrally concentrated spheroid with a relatively smooth, featureless morphology. The light profile suggests a significant bulge component. There may be a faint, diffuse disk, however there is no sign of spiral arms. The color profile suggests a population dominated by older stars, exhibiting a redder hue concentrated towards the central bulge, with a slight shift towards bluer colors in the outskirts. The overall structure implies an evolved system, potentially a lenticular or elliptical galaxy type, with limited ongoing star formation. There are no obvious signs of tidal features or major disturbances indicating recent or ongoing merger activity, though a minor interaction cannot be completely ruled out given the slight asymmetry in the outer regions.
