The galaxy appears as a centrally concentrated object with a generally smooth morphology. There's a noticeable bright central region, likely the galactic nucleus. The galaxy's color profile suggests a population of older stars, indicated by the relatively redder hue observed. There is a slight disc shape visible, indicating the likelihood of some rotation. There's a potential for minor disturbance, although not strongly defined. Any merger activity seems unlikely. The galaxy is fairly round, but shows a slight cigar shape. Overall, it seems to be an early-type galaxy.
