The galaxy presents a largely smooth morphology, appearing nearly circular in shape. The light distribution is relatively even, with a possible slight central concentration. The galaxy exhibits a predominantly yellow hue, suggesting an older stellar population and a low rate of ongoing star formation. There is a slight hint of bluer light in the outer regions, but it is faint. There is no obvious spiral structure or prominent dust lanes visible. The galaxy appears isolated and undisturbed, without any obvious signs of tidal interactions or merging activity.
