The galaxy presents an elliptical morphology, with a centrally concentrated brightness profile indicating a significant bulge component. The light distribution appears relatively smooth, suggesting an older stellar population dominates its composition. There is a slight asymmetry or subtle distortion in the outer isophotes, perhaps hinting at a past or ongoing minor interaction. The overall color is yellowish, consistent with galaxies dominated by older, redder stars. Star formation is likely occurring at a low rate within the galaxy.
