The galaxy presents a largely smooth, elliptical morphology, with minimal discernible spiral arm structure or prominent dust lanes. The central region exhibits a high concentration of light, suggesting a significant bulge component. The overall color is yellowish, indicative of an older stellar population and a relatively low rate of ongoing star formation. It appears mostly undisturbed, with no obvious signs of a major merger event or tidal disruptions. The galaxy appears slightly elongated but generally lacks a highly flattened disk-like structure. There may be minor disturbances evident, but they do not disrupt the smooth overall structure.
