The galaxy presents a generally smooth, elliptical morphology. Its color profile indicates a redder hue overall, suggesting an older stellar population and lower levels of ongoing star formation. The galaxy exhibits a relatively high degree of circularity in its overall shape. There is no immediately apparent evidence of a major merger or significant tidal disturbances, though there is a possibility of minor past interaction given the slight irregularity of the light distribution. Its estimated size is several kiloparsecs across.
