This galaxy presents as a somewhat amorphous, yellowish-white central region with an extended, diffuse halo of light. The color gradient indicates a population of older stars dominating the central bulge. It is not perfectly spherical, presenting a mild degree of elongation. There is some evidence of minor irregularity in its form, potentially suggestive of a previous or ongoing minor interaction with another celestial body, although a merger does not seem eminent. While there is no clear spiral structure, the slight bluer tint towards the outer edges suggests the presence of younger, hotter stars, possibly indicating some ongoing star formation. Overall, the galaxy appears relatively smooth and evolved.
