The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge. Its color profile exhibits a yellowish-orange hue, suggesting a stellar population dominated by older, cooler stars. There are no readily discernible spiral arms or significant dust lanes, contributing to its smooth appearance. The galaxy's shape deviates slightly from a perfect circle, exhibiting a degree of elongation. There is no evidence of major ongoing mergers or tidal disturbances, though subtle asymmetries might indicate minor gravitational interactions in its past. The absence of blue colors suggests a low rate of recent star formation. The galaxy appears relatively isolated within the observed field.
