The galaxy appears as a single, relatively smooth object with a distinct elliptical morphology. The central region exhibits a yellowish hue, indicating a possible older stellar population. This transitions outward to a slightly fainter, reddish-tinged halo. A potential disturbance in the morphology is implied, possibly due to a minor interaction or ongoing merger, and the slight asymmetry in the outer regions. There may also be a nearby smaller irregular object possibly interacting with the galaxy. The overall light distribution is somewhat concentrated, with the majority of the light emanating from the core and inner regions.
