The galaxy appears as a relatively compact, elliptical-like object with a smooth, diffuse light profile. A discernible bright central bulge or core dominates the galaxy's structure, exhibiting a yellowish-golden hue, suggesting an older stellar population. There are no clear indications of spiral arms or significant dust lanes. The overall shape is somewhere between round and elliptical. There are no obvious signs of any ongoing major merger activity or tidal disturbances, but there may be minor asymmetry or slight irregularity in the outer regions, possibly hinting at a past interaction or minor disturbance. Star formation appears to be low.
