The galaxy appears as a small, faint, elongated structure with a smooth light distribution. Its color profile suggests a predominantly older stellar population. The galaxy's overall shape indicates a spheroid or possibly an elliptical morphology. There is no strong evidence of spiral arms, active star-forming regions, or significant dust lanes, although the central region displays slightly bluer colors. It may be a disk galaxy with the view from the side. There do not appear to be signs of any major interactions or tidal disturbances.
