The galaxy presents a largely smooth, elliptical morphology. The central region exhibits a concentrated, bright core, potentially indicative of an active galactic nucleus or a high density of stars. There's evidence of a tidal interaction or merger, as suggested by the asymmetry and subtle distortions in the outer regions of the galaxy, with the core region being more compact. A slight extension is visible with hints of a tidal tail. The galaxy displays a reddish hue, implying an older stellar population and low ongoing star formation rate. The majority of the light appears to be emitted from a single bulge-like component, which is round. Some disturbance of the structure is seen, suggesting a minor disruption or merger.
