The galaxy presents as a centrally concentrated object with a smooth, diffuse light distribution. There is a slight ellipticity to its overall shape, appearing more "in between" round and elongated, but not cigar-shaped. No distinct spiral arms or bar structures are visible. The galaxy appears to be dominated by older stellar populations based on its yellow-reddish hue. There is no evidence of significant ongoing star formation activity. There is no obvious visual disturbance that would indicate a recent or ongoing major merger. A minor disturbance cannot be ruled out completely due to slight variations of the light profile, but it is unlikely.
