The galaxy presents as an elliptical morphology, demonstrating a relatively smooth light distribution. The central bulge is prominent, appearing bright and concentrated with a yellowish hue, suggestive of an older stellar population. The outer regions of the galaxy exhibit a gradual decline in surface brightness, appearing more diffuse and reddish, indicative of a fainter and potentially redder stellar population. There is a slight suggestion of a very faint disk feature, but the overall structure is dominated by the elliptical shape. The galaxy does not display any obvious signs of active star formation, major mergers, or tidal disturbances.
