The galaxy presents as a centrally concentrated, somewhat elongated object. The light profile suggests a relatively smooth distribution, transitioning from a bright core to a fainter, diffuse outer region. There is a subtle color gradient observable, with the central region appearing more red/yellow, suggesting a population of older stars, and the outer regions exhibiting a slightly bluer hue, possibly indicative of more recent or ongoing star formation. There is a hint of slight asymmetry or a minor disturbance in the outskirts, but the overall morphology is relatively undisturbed, suggesting a lack of recent major mergers. The galaxy has a lenticular or early-type spiral appearance.
