The galaxy appears to be a relatively smooth object, likely an elliptical galaxy or a lenticular galaxy with a dominant bulge. The light distribution is centrally concentrated, with the highest intensity at the core, gradually decreasing outwards. There is a slight elongation, which suggests that it may be more in between round and cigar shaped. It exhibits a yellow hue, indicating an older stellar population with a lower rate of star formation. There is a possible minor tidal disturbance visible, suggesting a past or ongoing minor merger.
