The galaxy presents as a relatively smooth, elliptical morphology. Its light profile appears concentrated and centrally bright, fading gradually outwards. No distinct spiral arms or significant dust lanes are discernible. The galaxy exhibits a yellow-orange hue, suggesting a stellar population dominated by older stars. The overall shape appears close to round with a slight elongation in one direction. There is no evidence of any major mergers or tidal disturbances. The galaxy's estimated size is a few kiloparsecs. Based on its color and morphology, the galaxy likely has a lower specific star formation rate.
