The galaxy presents as an elliptical morphology. Its shape appears cigar-like, significantly elongated along its major axis. The light distribution is smooth, lacking any prominent spiral arm structures or distinct features suggestive of ongoing major mergers. There is a concentrated, bright central bulge. The color gradient indicates a population of older stars, contributing to a redder overall hue. There is no obvious dust lane. There is no evidence of recent major interaction. It is a relatively large galaxy. The star formation rate is estimated to be relatively low.
