The galaxy exhibits a morphology that is neither entirely smooth nor strongly featured. It presents a generally elliptical shape, with the longer axis extending noticeably. There are no clear spiral arms or a well-defined disk structure. The central region appears brighter and has a yellowish-orange hue, possibly indicating an older stellar population. Surrounding this core is a more diffuse, fainter region with a bluer tint, potentially suggesting some ongoing star formation, although the rate appears relatively low. The light distribution suggests a somewhat disturbed or irregular shape, potentially influenced by a minor gravitational interaction. The overall color gradient shifts from redder at the core to bluer in the outer regions.
