The galaxy presents a predominantly smooth morphology, with a high degree of central concentration. Its overall shape appears nearly round to moderately elliptical. A distinct, though faint, extension or possible tidal tail is visible on one side, potentially indicative of an interaction or merger event in its past, or currently ongoing. The main body of the galaxy exhibits a color gradient, transitioning from a slightly reddish-yellow core to bluer outer regions. This might suggest an older stellar population centrally, with ongoing or recent star formation in the periphery. There is minimal evidence of strong spiral arm structures or prominent dust lanes within the galaxy's disk. Overall, the galaxy appears to be a relatively evolved system, possibly transitioning toward or already residing on the red sequence.
