This galaxy presents as a smooth, centrally concentrated object. The light profile appears to be dominated by an elliptical distribution, with a notable lack of distinct spiral arm structures or prominent dust lanes. A bright, unresolved core is visible, suggestive of a significant concentration of stars and potentially a supermassive black hole. The galaxy's overall color is relatively uniform, trending towards slightly redder hues compared to what would be expected of a strong star-forming galaxy. This implies an older stellar population. There are subtle variations in surface brightness throughout the galaxy's extent. The galaxy's overall shape appears roughly circular, with only a slight elongation. Based on these features, the galaxy's morphology is consistent with that of an elliptical or lenticular galaxy, likely possessing a relatively quiescent star formation rate.
