The galaxy appears to be an elliptical galaxy with a smooth, featureless morphology. It exhibits a centrally concentrated luminosity profile, with a diffuse halo extending outwards. The galaxy's color suggests a relatively old stellar population, indicating a low rate of on-going star formation. There are potential signs of a minor interaction or merger occurring within the galaxy. Overall, the galaxy appears relatively relaxed, with no strong evidence of a recent major merger or significant starburst activity. The galaxy's shape is generally in between round and cigar shaped. 
