The galaxy presents an overall elliptical morphology, elongated along its major axis. The central region exhibits a brighter, more concentrated luminosity, suggesting a significant stellar density. The galaxy's color profile appears relatively uniform, with a yellowish-white hue dominating the central bulge, transitioning to a slightly bluer tint at the outer edges. The smoothness of the light distribution across the galaxy indicates a relatively old stellar population, with little evidence of prominent spiral arms or significant dust lanes. There are no obvious signs of tidal interactions or major mergers in progress, though a slight asymmetry in the outer halo might indicate past interactions. The overall form is indicative of a relatively undisturbed, evolved galaxy residing at a redshift of approximately 0.135. The effective radius of the galaxy is estimated to be around 8 kpc. The inferred mass suggests a substantial system, likely a massive elliptical galaxy.
