The galaxy presents as a relatively compact, elliptical-like structure. It exhibits a smooth, featureless morphology with a somewhat diffuse boundary, suggesting an older stellar population and a lack of significant ongoing star formation. The overall color appears to be slightly yellow or golden, consistent with a dominant population of older, cooler stars. There is no obvious indication of spiral arms, dust lanes, or other prominent features typically associated with disk galaxies. There is a slight elongation visible, but not enough to classify it as a cigar shape. Some faint structures may be present, but none suggest strong tidal interactions or merging events. Overall the galaxy appears quite relaxed, suggesting a system that has evolved in isolation for a significant period of time.