This galaxy presents as a compact, moderately bright object. It exhibits a primarily smooth morphology with a concentration of light toward the center, indicative of a central bulge or nucleus. The color gradient suggests a relatively blue core transitioning to a redder halo, implying a potential mix of stellar populations, with younger, hotter stars concentrated centrally and older, cooler stars more prevalent in the outer regions. There appears to be some irregularity in the central structure. Overall, the galaxy's appearance is suggestive of a early-type spiral galaxy or a dwarf elliptical galaxy.
