The galaxy presents a generally smooth, elliptical morphology. It appears highly rounded with no obvious disk-like structure or spiral arms. The light distribution is concentrated towards the center, displaying a noticeable bulge. There are no signs of tidal tails, bridges, or other obvious features indicative of a recent merger event. The galaxy exhibits a yellow-reddish hue, suggesting a population dominated by older stars, with a potentially low rate of current star formation. There may be a slight asymmetry in the outer regions of the galaxy.
