The galaxy presents as a single, luminous object, with a relatively smooth, elliptical morphology. There is a central concentration of light that appears to be more intensely bright, suggesting a prominent galactic nucleus. The galaxy's color profile appears to be skewed towards the redder end of the spectrum. The overall form is generally rounded, with only a slight elongation, and there are no obvious signs of spiral arms or significant substructure visible. The galaxy does not seem to be undergoing any major merging events or showing strong tidal disturbances; it seems to be an isolated, relatively undisturbed system.
