The galaxy presents as a moderately bright object with a relatively smooth, diffuse morphology. It exhibits a nearly circular shape, suggesting a classification leaning towards elliptical or S0. There is a subtle hint of elongation, though not pronounced enough to categorize it as cigar-shaped. The color is generally uniform across the galaxy, appearing whitish, which might indicate an older stellar population dominating the light output, but the magnitude in the G band is high enough to suggest star formation is still present. There is no clear evidence of strong spiral arms or a prominent disk structure. No major mergers or significant tidal disturbances are visible. There may be a hint of a small disturbance in the structure but no major disturbance. The galaxy appears relatively undisturbed with little to no interaction with neighboring galaxies.
