The galaxy presents a generally smooth morphology, with a centrally concentrated, bright core exhibiting a yellow-orange hue. The light suggests an older stellar population dominates, indicative of minimal ongoing star formation. The overall shape appears to be somewhere in between a sphere and a disk. There is no obvious evidence of a spiral arm structure or significant dust lanes. The galaxy does not appear to be undergoing a major merger or strong tidal interaction with another galaxy, and there is no indication of a significant major disturbance or tidal tail. The approximate estimated size of the galaxy is around 10 kpc across.
