The galaxy presents a generally smooth, elliptical morphology, with a concentrated central bulge. The color gradient suggests a stellar population that is relatively old, exhibiting a yellowish-red hue within the core region. Fainter, bluer emissions are present along the outer edges of the galaxy, suggesting the presence of some younger stars, though they do not dominate the overall color profile. There is no significant evidence of spiral arms or a distinct disk structure. There do not appear to be any obvious signs of a major ongoing merger event, although minor irregularities in the outer halo regions cannot be ruled out, given image resolution. The galaxy exhibits a moderately round profile. Overall, the galaxy appears to be a relatively quiescent, evolved system with ongoing, though limited, star formation in the outer regions.
