The galaxy presents an elliptical morphology, elongated with a major axis significantly larger than its minor axis. It exhibits a smooth, featureless light distribution, lacking discernible spiral arms or distinct structures. The core is concentrated and intensely luminous, fading gradually outwards. The color gradient suggests a population of older stars within the central bulge, shifting toward redder wavelengths, with bluer hues present within the outskirts. The galaxy lacks any evidence of ongoing major merging events, however a faint disk may exist.