The galaxy presents as a relatively smooth, centrally concentrated structure. It exhibits a roughly elliptical morphology, appearing mostly 'in between' round and cigar shaped. The galaxy's core is bright and densely packed, suggesting a significant concentration of stars and possibly a supermassive black hole at its center.

There is a subtle color gradient present, with the central region appearing slightly yellowish-white, transitioning to a bluer hue in the outer regions. This could indicate younger star populations or ongoing star formation in the outskirts compared to an older stellar population in the bulge.

No distinct spiral arms or a prominent disk structure are readily discernible. There are no apparent signs of major mergers or tidal disturbances.
