The galaxy appears to be an elliptical type. The light distribution is relatively smooth and centrally concentrated, lacking any discernible spiral arm structure or prominent dust lanes. It exhibits a yellowish-red hue, suggesting a stellar population dominated by older, redder stars. The galaxy displays a moderate degree of roundness, with no obvious elongation or cigar-like shape. Indications of a possible merger event are present. There may be some form of disturbance to the galactic structure, but no major disturbance is indicated.
