The galaxy presents a somewhat elliptical morphology with a bright, concentrated central region. The radial light profile appears smooth, suggesting a dominant bulge component, possibly a Sersic profile. The color gradients indicate a central reddening, possibly due to older stellar populations and/or dust obscuration. The outer regions exhibit bluer colors, suggestive of ongoing or recent star formation. There is no strong evidence of spiral arms or a prominent disk structure. There may be some minor disturbances of the galaxy, or even some dust lanes near the core.
