The galaxy presents a generally elliptical morphology, appearing predominantly smooth in texture. The central region exhibits a high concentration of light, suggestive of a prominent galactic bulge. Moving outwards from the core, the luminosity gradually diminishes, forming a diffuse halo. Subtle colour gradients are discernible; the central bulge appears to exhibit a slightly yellowish hue, which may indicate an older stellar population. The outer regions transition to a more bluish tint, hinting at the presence of younger, hotter stars. The galaxy appears undisturbed, showing no significant signs of tidal interactions or major mergers.
