The galaxy presents as a well-defined, elliptical morphology. Its central bulge exhibits high luminosity with a yellowish hue, suggestive of an older stellar population. The disk is elongated, demonstrating a flattened spheroid shape. There is a smooth transition of luminosity from the core outwards. The disk appears relatively featureless, with no obvious spiral arm structure or dust lanes visible. The overall color gradient indicates a possible decline in star formation rates moving outwards from the central bulge, with bluer colors at the edges of the disk. The galaxy has a regular shape, showing no signs of major mergers or significant tidal distortions.
