The galaxy appears as a somewhat smooth, elliptical-like structure. It has a concentrated, luminous core which transitions into a more diffuse halo. The core region exhibits a yellowish-orange hue, possibly indicative of an older stellar population. Faint, greenish-blue tinges are visible in the outer regions of the galaxy, and there appears to be slight asymmetry in the disk. There is no definitive evidence of a strong spiral structure, but the disturbances suggest a possible interaction with another galaxy. 