The galaxy presents as a somewhat smooth, elliptical-like structure. The central bulge is a bright, concentrated region, exhibiting a yellowish-orange hue, suggesting an older stellar population. Fainter, blue-ish regions can be observed further out from the core, indicating regions of potential recent or ongoing star formation. The outer regions of the galaxy appear less defined and diffuse, fading into the background. There is a possible minor disturbance to the morphological structure, but the galaxy maintains a coherent overall form. It exhibits an apparent spheroidal shape with hints of elongation. There are no strong indications of spiral arms, but there is a slightly uneven distribution of the bluer star-forming regions in the outer disk.
