The galaxy exhibits a largely smooth morphology, with minimal discernible features suggestive of spiral arms or significant dust lanes. Its overall shape appears approximately round, with no strong elongation apparent. The color profile indicates a dominant population of older stars, suggested by the reddish-yellow hue, particularly concentrated toward the galaxy's core. A gradual decline in surface brightness extends outward from the central region, forming a diffuse halo. There are no obvious signs of ongoing major mergers or tidal disturbances, although a slight asymmetry cannot be ruled out due to the limitations of the image resolution. Star formation appears to be relatively quiescent.
