The galaxy appears to be a relatively smooth, elliptical system, exhibiting a predominantly spheroidal morphology. There is little evidence of spiral arms or significant disk structures. The light distribution appears centrally concentrated, with a gradual decrease in brightness towards the outer regions. There is a slight elongation in the morphology, as opposed to being perfectly circular. The galaxy exhibits a yellowish-white color, suggesting a population of older stars. The galaxy shows no signs of a recent major merger, though there might be some minor disturbances in the outer halo. There is also evidence of ongoing, albeit low-level, star formation within the galaxy.
