The galaxy presents as a relatively smooth, elliptical-like system with a noticeable bulge. It exhibits a centrally concentrated brightness profile, gradually decreasing in intensity outwards. The galaxy's color suggests an older stellar population, particularly within the central bulge, as evidenced by the yellow/red hue. There is a suggestion of a faint, extended disk component, as evidenced by the slight bluer/gray colored light, which is indicative of ongoing or recent star formation. The galaxy's overall shape is not perfectly round, showing a slight elongation, giving it an oval appearance. There is no obvious evidence of major spiral arms, strong dust lanes, or significant tidal disturbances that would indicate a recent major merger event, but instead, there are some minor disturbances that show a possible minor merger. The galaxy seems to be in a relatively relaxed state.
