The galaxy appears to be a relatively smooth, featureless system, likely an elliptical or lenticular galaxy. It exhibits a centrally concentrated brightness profile, with a gradual decline in luminosity outwards. The galaxy displays a subtle color gradient, transitioning from a bluer core to a redder halo. There is no obvious presence of spiral arms or dust lanes. The overall morphology suggests a system dominated by an older stellar population, with minimal ongoing star formation. The shape is somewhat rounded, with no significant elongation or tidal disturbances visible. Any potential merger activity seems minimal, as no major distortions are present.
