The galaxy appears as a singular, relatively smooth object. It exhibits a roughly circular morphology, with no obvious spiral arm structures or a distinct galactic bar. The light distribution appears concentrated towards the center, with a gradual decrease in intensity moving outwards. A slight elongation can be perceived, but the overall shape is predominantly round.

The color profile suggests a dominant population of older stars, inferred from its yellow and red tones. There is no noticeable presence of blue light, which would have indicated regions of active star formation. No signs of tidal tails, distorted shapes, or other indications of a recent major merger or significant gravitational interaction are visible. There seems to be a possible minor disturbance on one side of the galaxy in the form of a small amount of brighter light.
