The galaxy presents an elliptical morphology, though with subtle irregularities suggesting potential interactions or internal dynamics. Its color profile appears consistent with a redder population, indicating older stars. The galaxy's light is concentrated in a central region, with a gradual decrease in intensity towards its outer edges. Despite its predominantly smooth appearance, there are hints of disturbed structure, such as tidal features or minor asymmetries, indicating a possible merger event. The overall light distribution suggests a bulge-dominated system. There are also potential signs of merging or tidal features on the edges of the galaxy. 
