The galaxy appears as a fairly smooth, elliptical object. It exhibits a concentrated central bulge that gradually diffuses outward into a less defined halo. The galaxy's color profile suggests a population of older stars, with a dominant yellowish hue. There is no obvious indication of spiral arm structure or significant dust lanes. The overall shape appears mostly round, showing no significant elongation. There is no evidence of any major mergers or tidal disturbances affecting the galaxy's morphology. It appears to be a relatively undisturbed, evolved system.
