The galaxy presents with a relatively smooth, elliptical morphology. It exhibits a centrally concentrated bulge, characterized by a yellowish-orange hue, which suggests a population of older, redder stars. The galaxy appears to be moderately luminous. The system may be undergoing a minor interaction or disturbance, evident from the asymmetry. A blue region appears to be extending from the galaxy, possibly indicative of an area of active star formation. 
