The galaxy presents a smooth, elliptical morphology. It exhibits a notable elongation, appearing cigar-shaped rather than perfectly round. There is no clear evidence of spiral arm structure or significant dust lanes. The color profile is relatively uniform across the galaxy, with a tendency toward redder hues. This color and smooth morphology suggests a population dominated by older stars. There does not appear to be any major tidal disturbance or clear signs of an ongoing merger event. Based on its red color, the galaxy appears relatively evolved, with moderate star formation.
