The galaxy appears as a centrally concentrated object with a relatively smooth morphology. It exhibits an elliptical shape, appearing somewhat flattened rather than perfectly spherical. The light is dominated by a yellowish-white hue, suggesting an older stellar population. There are no obvious spiral arms, bars, or distinct dust lanes visible. A slight elongation is noticeable, implying a possible cigar-like shape. No signs of major merging events are present. Subtle disturbances may exist, but are not prominently observed. Overall, it presents a regular structure indicative of a galaxy undergoing quiescent evolution.
