This galaxy presents as an elliptical or lenticular type, exhibiting a generally smooth morphology without prominent spiral arms or a well-defined disk structure. The light distribution appears centrally concentrated with a gradual decrease in intensity outwards. It has a moderate degree of roundness. There are no signs of tidal tails, disrupted morphology, or other indications of recent major merger activity. It exhibits a reddish-yellow hue, suggesting a population dominated by older stars. The overall color profile implies relatively low levels of current star formation.
