The galaxy presents a generally smooth, elliptical morphology with a concentrated central bulge. The galaxy appears largely spheroidal with a noticeable lack of distinct spiral arm structures. There may be a slight flattening giving it an intermediate shape between round and elongated. The core exhibits a brighter, more intense luminosity suggestive of a high density of stars. Fainter extended regions are visible around the main body, indicating a possible halo or tidal features from previous interactions. The color distribution suggests a population of older stars dominating the central region, with a transition to slightly bluer colors in the outer regions, possibly indicating some ongoing star formation. There appear to be some minor disturbances in the galaxy's overall structure.
