This galaxy presents as a centrally concentrated object with an ellipsoidal morphology. The light distribution appears smooth, with no prominent spiral arms or distinct disk structures readily visible. There appears to be little to no dust obscuration visible within the main body of the galaxy. The color profile of the galaxy is predominantly yellow. This is consistent with a stellar population dominated by older stars with lower ongoing star formation. The roundness of the galaxy appears between round and cigar shaped, closer to a round form. There appears to be no signs of major disturbance, such as tidal tails. This assessment suggests that this galaxy does not have a large star formation rate.