The galaxy appears to be a relatively luminous elliptical or lenticular system. It exhibits a smooth, centrally concentrated light profile, with a bright, yellowish core that suggests an older stellar population dominating the central regions. The galaxy appears generally featureless, with no distinct spiral arms or prominent dust lanes visible. There is a slight elongation of the galaxy's shape, with a ratio of about 4:3 between the semi-major and semi-minor axes. The lack of strong blue emission suggests a relatively low ongoing star formation rate. The overall morphology indicates a relatively evolved system. There appears to be little to no evidence of interactions or major mergers in its recent history.
