The galaxy appears to be an elliptical galaxy, exhibiting a smooth, featureless morphology. It has an overall round shape, but it also has an elongated structure, somewhere between round and cigar shaped. The light is concentrated towards the center, indicating a high stellar density in the core. The color profile suggests a relatively older stellar population, with a redder hue in the outer regions, likely due to the presence of older, cooler stars. There is no evidence of spiral arms or significant dust lanes, further supporting the classification as an elliptical galaxy. Additionally, there is no evidence of any major ongoing merger or tidal disturbance. The estimated size of the galaxy is a few kiloparsecs.
