The galaxy presents as a centrally concentrated, luminous object with a smooth, largely featureless appearance. The core region exhibits a bright, yellowish-white hue, indicating a concentration of older stellar populations and potentially ongoing star formation. The galaxy's radial profile suggests a gradual decrease in surface brightness outwards from the core, transitioning to a reddish-orange color in the outer regions. The overall shape appears somewhat elliptical, leaning towards a more spherical morphology rather than a highly flattened disk. There is no obvious presence of spiral arms or prominent dust lanes. There is no signs of any major merger event.
