The galaxy presents as a centrally concentrated, relatively smooth system. The light profile suggests a dominant bulge component, with a notable decrease in intensity moving outwards. The overall shape is approximately elliptical, showing a slight elongation. There is no clear evidence of spiral arm structure or a prominent disk from this view. Color gradients are subtle, but a slight reddening appears to be present in the central region, potentially indicating an older stellar population compared to the outer regions. No significant signs of recent major merger activity are observed, such as tidal tails or disrupted morphology. The absence of obvious dust lanes or prominent star-forming regions suggests a relatively passive star formation history.
