The galaxy presents as an elliptical morphology, characterized by a smooth, centrally concentrated light distribution. The core region exhibits a yellowish hue, potentially indicative of an older stellar population. The outer regions transition to a bluer color, implying a modest level of recent star formation. There is no apparent disk structure, spiral arms, or bar. No significant tidal features or signs of major mergers are observed, though a slight asymmetry might suggest minor interaction. The galaxy appears relatively isolated.
