The galaxy presents as a relatively smooth, elliptical structure with a concentrated central bulge. It exhibits a dominant yellowish hue in the core, transitioning to a bluer tint in the outer regions. The overall morphology suggests an evolved system, potentially undergoing minimal ongoing star formation. There appears to be little evidence of spiral arms or significant dust lanes; the galaxy appears largely featureless, implying a lack of recent major mergers. The structure is mostly round, with only a slight flattening. No signs of significant gravitational disturbance or interaction with neighboring galaxies are immediately apparent.