The galaxy appears to be an elliptical galaxy, exhibiting a centrally concentrated luminosity profile that gradually fades towards the outskirts. The central region of the galaxy displays a yellowish-white color, suggesting an older stellar population. Moving outward from the core, a subtle bluish hue becomes more apparent, possibly indicating the presence of a younger stellar population or some star formation in the outer regions. There are no discernible spiral arms or a distinct disk-like structure. The galaxy appears relatively smooth with a mostly regular morphology, but there is some slight distortion in the halo, which could be indicative of a minor disturbance, possibly due to a past merger event. 
