The galaxy presents as a moderately luminous, elliptical type. Its morphology appears largely smooth and spheroidal. The core region exhibits a concentrated luminosity, transitioning outwards to a fainter halo. Color gradients are subtle but visible, with the core showing a yellower hue suggestive of an older stellar population, while the outer regions show more traces of blue, potentially indicating some ongoing star formation, however limited. There is no obvious sign of spiral arm structure or a prominent disk. The overall form is well-defined and lacks any major disturbances or tidal features indicating past or ongoing merger events. The image is not high resolution, so internal structures cannot be analyzed in great detail.
