The galaxy presents as a largely smooth, elliptical-like structure. It exhibits a concentrated central bulge which appears more luminous and yellowish in color. A slight elongation is observed, suggesting a deviation from a perfectly circular morphology. No prominent spiral arms, dust lanes, or distinct star-forming regions are readily apparent. The galaxy appears relatively undisturbed, with no major signs of ongoing mergers or tidal interactions. Its color suggests an older stellar population dominated by redder stars. Overall, this galaxy appears to be a relatively massive and evolved system, likely with a suppressed star formation rate.
