The galaxy presents as a centrally concentrated object with a relatively compact morphology. There is evidence of a disk structure, viewed at a shallow angle, possibly near edge-on. The central region displays a bright, concentrated core. The galaxy exhibits a color gradient, transitioning from a yellowish core to a slightly bluer disk component. Based on this color information, the central core may host an older stellar population compared to its disk. Hints of disturbance are present, but not overwhelming. This leads to a classification of either a typical undisturbed elliptical galaxy or a spiral galaxy with a large central bulge.
