The galaxy presents a generally smooth and elliptical morphology. The light is concentrated towards the center, with a distinct but relatively small, bright core region. The galaxy shape is elongated, deviating slightly from a perfect circle towards a more cigar-like form. There is a slight color gradient, appearing more yellow/red towards the center, fading to a bluer hue towards the edges, although these color differences are subtle. No clear spiral arm structures or distinct dust lanes are visible. There is no strong evidence of major tidal disturbances or ongoing mergers, although some minor irregularities in the outer regions cannot be entirely ruled out. The galaxy exhibits a relatively low star formation rate, consistent with the lack of prominent blue regions often associated with young, hot stars.
