The galaxy presents as a largely smooth, elliptical morphology. The central region exhibits a bright, concentrated core, possibly indicative of an active galactic nucleus or a dense stellar population. Moving outward from the core, the light profile gradually diminishes. There is evidence of a subtle color gradient, shifting from a warmer, yellower hue in the central bulge to a cooler, bluer tinge in the outer regions. This color variation might suggest differing stellar populations, with older, redder stars concentrated in the center and younger, bluer starsPopulations distributed more peripherally, as well as differing levels of dust. There is no definitive spiral arm structure visible, nor any obvious signs of major disturbances or ongoing merger activity within the galaxy. Faint irregularities or disturbances might be taking place in the outer areas. The overall roundness and lack of significant features indicate that the galaxy is likely a relatively relaxed system, in terms of galactic structure. The galaxy is relatively compact in size.
