The galaxy presents as a flattened spheroid, appearing as a smooth distribution of light with a high degree of central concentration. The overall color is predominantly white to bluish-white, suggestive of a population of relatively young, hot stars. The light distribution fades gradually toward the edges, indicating a lack of sharp boundaries. There is a subtle elongation, and the overall structure is mostly undisturbed, without any obvious signs of strong tidal interactions or recent major mergers, though there are slight disturbances. This suggests a galaxy with low recent merging activity.
