The galaxy presents as a generally smooth, elliptical-like object with no obvious spiral arm structure. The core appears bright and concentrated, exhibiting a yellowish-white hue. The overall light distribution suggests a centrally concentrated luminosity profile. There is a subtle color gradient, with the central region appearing slightly bluer than the outer halo. The galaxy shows a slightly elongated form, not perfectly spherical, tending toward a more disk-like appearance when taking the fuzzier halo into account. There is no immediately apparent evidence of significant tidal interactions or major merging events, although a minor disturbance cannot be ruled out based on the available imagery. Star formation appears minimal based on the color indices, suggesting an older stellar population dominating the light emission.
