The galaxy presents a predominantly smooth and rounded morphology, suggesting a classification as an elliptical galaxy. Its color profile indicates a reddish hue, implying a population of older, redder stars and a relatively low rate of ongoing star formation. There is minimal evidence of a disk structure or spiral arms. No prominent features are observed such as tidal tails, suggesting that there are no major disturbances or merger activity presently occurring, though there are some indications of a minor disturbance. The galaxy exhibits a concentrated central region.
