The galaxy presents as a relatively smooth, elliptical-like structure. The core exhibits a bright, concentrated luminosity, suggesting a high density of stars and potentially a supermassive black hole actively accreting matter. There's an extended halo surrounding the central region, its light gradually fading into the background. Faint and diffuse spiral arms appear to originate from the central bulge, however they are not well defined. The color gradient transitions from a warmer, yellower hue in the core to a cooler, bluer tint in the outer regions of the disk. The morphology suggests a mature system where star formation is present, yet declining. There appears to be no signs of ongoing major mergers or tidal disturbances in the immediate vicinity.
