The galaxy presents as a relatively smooth, elliptical-like structure. It appears moderately luminous, with a concentrated central region that graduates outward into a less defined halo. The overall shape is close to circular, exhibiting minimal signs of strong tidal disturbances or asymmetries. The light distribution seems uniform, with a slight color gradient from a yellow/orange center to a redder periphery, possibly indicating differences in stellar populations and age. Evidence of any spiral arm structure or distinct dust lanes is absent. There may be some small features or interactions happening in the galaxy.
