The galaxy presents an elliptical morphology, with a smooth, diffuse light distribution. Its shape is elongated, appearing somewhat cigar-shaped rather than perfectly round. The color gradient suggests a predominantly older stellar population, concentrated towards the galaxy's center. There may be evidence of a weak disk with blue stars present, but this requires further examination. No significant spiral arm structure or prominent dust lanes are apparent. The overall structure indicates a system that has likely undergone significant relaxation, lacking the irregular features typically associated with recent major mergers. The galaxy exhibits a reddish color index, suggesting it is a relatively quiescent galaxy with low ongoing star formation. There is a possible indication of minor disturbance; however, no distinct tidal features or signs of major interaction are observable.
