The galaxy presents as a slightly elongated, elliptical-like structure. A central bulge region appears with a bright, concentrated luminosity, suggesting a high density of stars. Moving outward from the central bulge, the light diminishes gradually, forming a diffuse halo. The color profile indicates a predominantly older stellar population, judging by the yellowish-orange hue dominating the galaxy's core and extended regions, with hints of bluer light in the outer edges. There's no clear evidence of spiral arms, indicating this is likely not a spiral galaxy. A somewhat irregular shape is observed, but it doesn't display any signs of ongoing major mergers or tidal disturbances. The overall texture is relatively smooth, suggesting a dynamically settled system that isn't currently experiencing a high rate of star formation. The galaxy displays a moderate inclination relative to our line of sight.
