The galaxy presents as a centrally concentrated elliptical structure with a relatively smooth, featureless appearance. There is a lack of prominent spiral arms or other distinct features. The light appears to be dominated by older stellar populations as indicated by the yellow-orange hue of the central bulge, with the outer regions subtly fading into a less intense glow. The axial ratio suggests a somewhat elongated shape but not highly flattened. There is no obvious indication of tidal disturbances, ongoing major mergers, or significant star formation activity. The galaxy appears relatively isolated and undisturbed.
