The galaxy presents as a relatively smooth object, exhibiting a near-spherical morphology with a slight deviation towards an elliptical shape. There is no strong indication of distinct spiral arms or a well-defined disk structure. The light distribution is centrally concentrated, with a gradual decline in surface brightness towards the outer regions. Faint hints of some structure can be seen at the edges but are not distinct enough to be described as any sort of specific feature. There is no obvious presence of ongoing major merger activity or significant tidal disturbances. The overall color appears to be subtly yellow-reddish, potentially indicating an older stellar population with relatively low ongoing star formation.
