The galaxy presents as a relatively smooth, elliptical or lenticular structure. The light is concentrated towards the center. There is a noticeable color gradient, trending from blue-green at the core to a slightly redder hue in the outer regions. This could indicate the presence of younger, hotter stars in the central region. The overall shape is mostly round, with only slight elongation. There is no apparent spiral structure or significant dust lanes. The lack of significant disruption suggests that the galaxy has not undergone a major merger recently. The estimated size is about 3.5 kpc, so it is a relatively small galaxy. The estimated star formation rate suggests this galaxy is forming very few stars.
