The galaxy appears to be an elliptical type, characterized by a smooth, concentrated light distribution. Its shape is generally elongated, but not highly so. There is no evidence of spiral arms or a prominent disk structure. The color gradient suggests an older stellar population, with a yellowish-white hue dominating the central region, indicating a lack of significant ongoing star formation. No signs of active galactic nuclei or major disturbances are readily apparent, although subtle signs of minor interaction cannot be ruled out based on the image alone. The galaxy's estimated size indicates a modest scale.