This galaxy exhibits a generally smooth morphology, with a slight elongation that suggests it is not perfectly spherical, but rather somewhat in between round and cigar-shaped. There are subtle hints of internal structure, possibly indicating a disk component but the galaxy is primarily composed of a smooth distribution of stars. There appears to be some minor disturbance, perhaps due to a past interaction, but the overall structure is largely undisturbed. The color profile indicates a mature stellar population, leaning towards redder hues, which corresponds to a relatively low rate of star formation. The galaxy appears fairly massive.
