The galaxy presents a smooth, elliptical morphology. Its light profile suggests a fairly uniform distribution with a slight concentration towards the center. There are no readily discernible spiral arms or distinct features, such as prominent dust lanes or star-forming regions. The overall color appears relatively uniform, skewed towards warmer tones, suggesting a population dominated by older stars. The galaxy exhibits a subtle elongation, not perfectly spherical, leaning toward a slightly cigar-like shape. It shows subtle signs of a potential minor disturbance, though a major merger is unlikely based on the observed morphology.
