The galaxy presents a largely featureless, smooth morphology. It appears elliptical in shape, exhibiting a high degree of roundness, and no apparent spiral arms or bar structures are visible. The galaxy shows a concentrated central bulge, with light intensity decreasing gradually towards the outer edges. The light distribution suggests a relatively homogenous stellar population, primarily older stars, contributing to its overall yellowish-red color. There's no significant evidence of on-going major merging activity. The overall color suggests that star formation is not currently a dominant process, though some minimal star formation cannot be ruled out.
