The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a concentrated central bulge that appears yellowish, suggesting a dominant population of older stars. Moving outwards from the core, the galaxy's color gradually shifts towards a redder hue, indicating an aging stellar population within the outer regions. The overall shape appears to be somewhat round. There is no visible evidence of spiral arm structures or significant dust lanes. The galaxy displays no signs of a recent or ongoing major merger event. Overall, this galaxy appears to be a mature system with a subdued star formation rate.
