The galaxy presents as a moderately luminous object, appearing nearly round in shape. It exhibits a generally smooth morphology with some subtle features, but no immediately obvious spiral arms or bar structure. The central region is distinctly brighter, suggesting a concentrated nucleus, possibly indicative of an actively star-forming region or an active galactic nucleus, though the resolution limits a definitive determination. There are some indications of minor disturbances in the galaxy's structure, but its overall shape suggests it is not undergoing a major merger. The galaxy is more or less of average mass, with evidence of ongoing low level star formation. Color gradients are observed, shifting from a slightly bluer central region to redder outskirts.
