The galaxy presents as a relatively smooth, elliptical-like structure. A bright, concentrated central bulge dominates the morphology, gradually fading into a more diffuse halo. The color profile suggests a mixture of stellar populations; the core region exhibits a bluer hue, potentially indicating ongoing or recent star formation activity, while the outer regions display a redder tint, indicative of older, redder stars. There's a subtle suggestion of a disk-like structure, but it's not sharply defined, mostly an intermediate rounded shape. Overall the galaxy seems fairly isolated with no significant signs of tidal interactions or major mergers in its recent past. Small, possibly minor disturbances are hinted at from the light distribution. The galaxy is not particularly compact or diffuse but with an estimated effective radius of 5 kpc is fairly normal for this type.
