The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge. The core exhibits a yellowish-orange hue, suggestive of an older stellar population. Surrounding the core is a fainter, greenish halo, potentially indicating the presence of younger stars or ongoing star formation, although the smoothness suggests a relatively low star formation rate overall. There is slight evidence of a minor disturbance of some kind as the shape is not perfectly round. The galaxy does not appear to be undergoing a major merger.
