The galaxy presents as a relatively smooth, centralized object. It exhibits a centrally concentrated light profile, appearing nearly round in shape. There is a general lack of distinct features, such as spiral arms or prominent dust lanes, suggesting a more evolved or quiescent morphology. The color profile appears to be dominated by light in the redder wavelengths, with little evidence of significant blue light indicative of recent star formation. The galaxy shows no clear signs of any major disturbance or ongoing merger activity. It's light spans approximately 3 kpc.
