The galaxy presents as a relatively compact object with a notable central bulge. It exhibits a smooth, somewhat elliptical morphology, with a high concentration of light towards the core, transitioning into a less defined, more diffuse outer region. The overall color appears to be yellowish-white, which is consistent with an older stellar population. There is faint evidence of possible disk-like structure or spiral arms, but the image resolution is limited. Slight disturbances may be present, but there is no clear signs of a major ongoing merger event.
