The galaxy appears as a relatively smooth, centrally concentrated object. Its overall morphology suggests an elliptical or lenticular classification, showing a largely spheroidal shape with minimal visible disk structure. There is no discernible bar or spiral arm structure. The light profile exhibits a distinct concentration towards the center, gradually fading into the surrounding space. The core region appears slightly reddish or yellowish, which could suggest a higher concentration of older stars and dust absorption. There is a hint of green in the outer regions of the galaxy. There appears to be no evidence of any major ongoing merger events, tidal tails, or strong gravitational disturbances.
