The galaxy presents as an elliptical morphology, characterized by a relatively smooth and centrally concentrated luminosity profile. The central region exhibits a yellowish hue, suggesting an older stellar population and minimal ongoing star formation within this core. Moving outward from the core, there's a gradual transition towards a more diffuse, reddish-tinged halo. The overall shape appears close to round, with a slight elongation that could indicate a minor triaxiality. There is no apparent disk structure or prominent spiral arms, nor is there any visual evidence of a recent major merger or significant tidal disturbances. There is potentially a very minor disturbance.
