The galaxy presents as a somewhat elongated, elliptical form, with a smooth, relatively featureless light distribution. The core region exhibits a strong concentration of luminosity, appearing significantly brighter than the surrounding areas. There is a gradual decline in surface brightness moving outward from the center toward the galaxy's edges. Faint extensions or tidal features are not readily apparent in this image, suggesting it is relatively undisturbed. The color profile indicates a generally redder overall hue, potentially indicative of an older stellar population and diminished ongoing star formation. The galaxy displays a moderate degree of ellipticity, appearing more cigar-shaped than circular. There are no prominent spiral arm structures visible.
