The galaxy exhibits a generally elliptical morphology, appearing somewhat flattened. It presents a smooth and featureless appearance, lacking distinct spiral arms or prominent dust lanes. The light distribution indicates a centrally concentrated bulge that gradually fades towards the outer regions. The color profile reveals a relatively redder hue overall. This color suggests an older stellar population and possibly lower rates of ongoing star formation activity within the galaxy. The estimated size indicates that it is a smaller galaxy. There may be some minor disturbance within the galaxy.
