The galaxy presents a generally smooth morphology, with a slight elongation. The shape appears to be somewhere between round and cigar-shaped. There is a faint, diffuse disk or other feature. It does not seem to show strong evidence of tidal disturbances or a major merger event. The object presents colors across the G, R, and Z bands, appearing bluish-white in the inner regions and gradually yellowing towards the outer edges. This color gradient might suggest a difference in stellar populations, with younger, bluer stars concentrated toward the core, and older, redder stars dominating the periphery. Overall, the galaxy appears to be a relatively massive system, exhibiting moderate levels of star formation.
