The galaxy appears to be a relatively small, faint, and somewhat irregular system. It exhibits a bright central region, potentially a nucleus or bulge. The light profile is relatively smooth although there are some disturbances in the shape. Evidence of a disk component is potentially present but not clearly defined. There are also no strong indications of spiral arm structures. A slight tidal tail or distortion is visible on one side, potentially indicative of a minor interaction or past merger event. The color distribution suggests some variation in stellar populations, with bluer regions, particularly near the outer edges, implying recent star formation activity, and a redder central region indicative of older stellar populations.
