The galaxy presents a relatively smooth and centrally concentrated morphology. It exhibits a generally elliptical shape, appearing mostly round with a slight hint of elongation. The core region displays a yellowish hue, suggesting a population of older stars and a reduced rate of ongoing star formation. Surrounding the core, there is a more diffuse outer region showing subtle gradients in color, shifting towards slightly bluer tones, possibly indicating the presence of younger stellar populations within a disk-like structure. There is no obvious presence of spiral arms or major distortions indicative of recent mergers. The galaxy appears relatively isolated, with no visually apparent companion galaxies or tidal features in its immediate vicinity.
