The galaxy presents as an elliptical-like structure, exhibiting a smooth morphology. It appears to be moderately luminous, with a bright, concentrated central bulge that transitions into a less defined, diffuse halo. The color gradient suggests an older stellar population dominating the bulge, indicated by its reddish-orange hue. Fainter, bluish-white regions are observed in the outer areas, potentially indicating some degree of ongoing, though limited, star formation within its disk-like component. There is a slight elongation of the structure, suggesting it may not be perfectly spherical, possibly leaning more towards an oblate spheroidal shape. A subtle asymmetry is present, hinted by a slight warping or tidal disturbance in the outer regions, possibly indicating minor interactions with surrounding structures or a past merger event.
