The galaxy presents as a centrally concentrated, smooth system. It appears to be relatively elliptical in shape, though not perfectly round. There is a lack of discernible spiral arm structure or prominent dust lanes. The central bulge region exhibits a higher surface brightness than the surrounding disk or halo. Color gradients appear subtle, with a generally blue-white hue towards the center, fading to a more yellow color in the outer regions. This color distribution suggests a potential decrease in the proportion of younger, hotter stars toward the galaxy's periphery. There are no obvious signs of ongoing major mergers or significant tidal disturbances, although minor irregularities cannot be ruled out at this resolution. Based on these observations, the galaxy is likely an early-type spiral or S0 galaxy with suppressed star formation.
