The galaxy presents as a relatively compact object. Its morphology appears largely smooth and spheroidal, exhibiting a notable concentration of light towards the center. There is a suggestion of a faint, diffuse halo extending beyond the bright core, though the image resolution limits detailed analysis. The color profile indicates a bias towards redder wavelengths, particularly in the central region, transitioning to slightly bluer hues at the periphery. This color gradient suggests a potential gradient in stellar populations, with older, redder stars dominating the core and a younger, bluer population in the outer regions. There is a hint of possible tidal disturbance, although it is difficult to determine from this image alone.
