The galaxy presents as a centrally concentrated, relatively smooth structure with a generally elliptical morphology. The central region exhibits a yellowish-white hue, suggesting an older stellar population. There is a very slight elongation, but its overall shape is largely round. The edges of the galaxy fade gradually, suggesting a diffuse halo or envelope of stars. There is a hint of redder tones on one side of the galaxy, possibly indicating regions of ongoing star formation, or perhaps simply dust attenuation. No obvious spiral arms or distinct features are discernible at this resolution. The galaxy appears to be relatively undisturbed, with no significant signs of tidal interactions or mergers.
