The galaxy presents a flattened, elliptical morphology, with a smooth, centralized concentration of light suggesting a prominent bulge. A faint disk may be present, but it appears tightly wound. The core exhibits a yellowish hue, possibly indicating a population of older stars. The outer regions of the galaxy show a gradual decrease in brightness with a bluer tint, which might be due to the presence of younger stellar populations or ongoing star formation, albeit at a low rate. There are no strong indications of spiral arm structures or significant dust lanes visible in the image, though some minor irregularities exist. Based on its shape and color profile, this galaxy is likely an intermediate-type spiral galaxy, possibly transitioning towards a lenticular form, or perhaps an elliptical galaxy with ongoing low levels of star formation. There appears to be a tidal disturbance.
