The galaxy appears as a centrally concentrated, moderately luminous system with a smooth, featureless morphology. The light profile is relatively diffuse, showing a gradual decrease in intensity from the core outwards. The color gradient suggests a population dominated by older stars, as indicated by the reddish-yellow hue, especially concentrated towards the center. There is little evidence of spiral arms, dust lanes, or prominent star-forming regions. The overall shape is slightly elongated but generally round. There is no obvious sign of tidal disturbances or ongoing merger activity, with the galaxy appearing relatively isolated and undisturbed. There appears to be an object to the upper left, which has a bluish tint, which may be interacting with the galaxy. 
