The galaxy presents as a relatively smooth, centrally concentrated object, potentially an elliptical or lenticular galaxy. Its overall shape appears moderately elliptical. The core of the galaxy exhibits a bright, yellowish-white hue, indicating a population of older stars. This central region transitions into a less concentrated, dimmer outer region. There is a subtle color gradient extending outward from the core. The outer regions of the galaxy appear slightly bluer, possibly indicative of some younger stellar populations or recent, though minimal, star formation activity. No distinct spiral arms or prominent dust lanes are visible. The galaxy seems relatively isolated, showing no signs of major ongoing merger activity or tidal disturbances, though there is a very faint, small object nearby which could be indicative of minor disturbance.
