The galaxy appears as a relatively smooth, centralized concentration of light. It exhibits a generally elliptical morphology, displaying minimal evidence of spiral arm structures or significant disk features. The light distribution is fairly even across the galaxy, with a gradual falloff in intensity from the core to the outer regions. There are subtle color variations across the galaxy's surface, with the central region showing a slightly bluer hue compared to the more reddish outskirts. No prominent dust lanes or active star-forming regions are immediately apparent. There seems to be no strong signs of recent or ongoing major mergers, though some slight irregularities in the outer edges could suggest minor interactions or disturbances. The overall form seems to be of a quiescent system with the possibility of limited star formation activity.
