The galaxy appears to be an elliptical galaxy, exhibiting a smooth, relatively featureless morphology. Its overall shape is more elongated than circular, tending toward an "in-between" shape rather than perfectly round or cigar-shaped. There is no discernable disk component or spiral arm structure. The galaxy presents a concentrated central bulge that gradually diffuses outwards with no strong evidence of significant dust lanes or active star-forming regions within the visible spectrum. There is a suggestion of only minor disturbances, hinting at the possibility of a past minor merger event but generally appearing isolated and undisturbed. The core is a yellow color suggesting a population of older stars.
