The galaxy presents as a generally smooth, elliptical-like structure with a concentrated central bulge. The light profile appears relatively uniform, lacking prominent spiral arms or distinct morphological features. The color gradient suggests a population of older stars, as indicated by the reddish-yellow hue of the core. There may be signs of a minor disturbance in the galaxy's morphology. A small, reddish secondary source is visible, possibly indicating an ongoing or past merger event. The galaxy exhibits evidence of moderate star formation activity.
