The galaxy presents as a relatively smooth, elliptical morphology. It exhibits a concentrated central bulge, with luminosity gradually decreasing outwards into a diffuse halo. Color gradients suggest a likely population of older stars, with a yellowish to reddish hue dominating the central regions and extending into the surrounding halo. The galaxy shows no obvious signs of spiral arms or active star formation regions. There is no evident dust lane or significant morphological disturbance indicative of a recent merger event. The general roundness indicates an elliptical classification rather than a disk-dominated spiral galaxy. There appears to be minor asymmetry in the outer halo, which could be the result of gravitational interactions or past accretion events, but the overall impression is of a well-defined, relaxed system.
