The galaxy presents as a generally smooth structure, exhibiting a dominant central bulge. The light distribution appears concentrated toward the core, fading gradually outwards. There is a hint of disk-like morphology, but the bulge component seems to contribute significantly to the overall luminosity. Weak asymmetrical features suggest there could be ongoing interactions or minor disturbances. The color profile indicates a relatively older stellar population, with reddish hues more apparent across the galaxy, suggestive of lower current star formation activity. The morphology could be classified as somewhere between elliptical and early-type spiral.
