The galaxy presents a generally smooth and rounded appearance. Its core region exhibits a bright, concentrated luminosity, with a yellowish-white hue, suggesting a significant population of older stars. The overall color profile trends towards redder wavelengths, potentially indicative of an elliptical morphology or a spiral galaxy with a dominant bulge component. Faint extensions are potentially visible indicating the presence of a faint galactic halo. There are no obvious signs of ongoing major merging activity or strong tidal disturbances. The absence of pronounced spiral arms or dust lanes suggests it is not a vigorously star-forming galaxy.
