The galaxy appears to be a relatively smooth, elliptical or lenticular type. Its light profile suggests a centrally concentrated bulge component, decreasing outwards. It appears to be generally well-defined. There's a subtle color gradient, transitioning from a yellower core region to slightly bluer outer edges. It does not seem to have any significant spiral arm structure or prominent dust lanes. The galaxy appears to be isolated, showing no immediate signs of ongoing major merger activity or tidal disturbances.
