The galaxy presents as a relatively compact object with a smooth, concentrated morphology. Its central region exhibits a yellowish hue, suggesting an older stellar population. A gradual decline in color and intensity extends outwards from the core, transitioning to a bluer periphery. This color gradient could indicate ongoing star formation in the outer regions, albeit at a lower rate. The galaxy appears largely undisturbed, with no obvious signs of tidal features or major mergers. However, there may be very minor asymmetric features along the outskirts. The overall shape approximates a flattened spheroid, presenting close to face-on with little observed disk structure.
