The galaxy presents a generally smooth morphology, with a dominant spheroidal component. Its color profile exhibits a central concentration of light, appearing more yellow or golden, suggestive of an older stellar population. Moving outward from the core, the color gradually shifts to a bluer hue, indicating the presence of younger stars. The overall shape of the galaxy is elongated, with the longest axis notably exceeding the shortest, indicating a non-circular appearance. There is no readily apparent evidence of strong spiral arm structure or a distinct disk. Slight irregularities in the outer regions might hint at minor disturbances, but the galaxy appears mostly undisturbed. Overall, this galaxy likely possesses a substantial mass.
