The galaxy presents as a largely featureless, elliptical morphology with a smooth light distribution. The core region is bright and concentrated, emitting a yellowish light that suggests an older stellar population and a lack of significant ongoing star formation within the central region. The outer regions of the galaxy exhibit a gradual decrease in luminosity with no apparent spiral arm structure or prominent dust lanes. There are hints of a slight disk-like structure. The overall roundness of the galaxy is evident, with only minor deviations from a perfect ellipse. No major signs of a recent merger event or tidal disturbances are visible in the galaxy's structure. The galaxy appears relatively isolated.
