The galaxy presents as a luminous, concentrated spheroid with a slightly elongated morphology. Its central region exhibits a high surface brightness, indicating a dense concentration of stars. Moving outwards from the core, the luminosity gradually decreases, transitioning into a more diffuse halo. There is no discernible spiral arm structure or significant dust lane obscuration visible. The color profile appears relatively uniform across the galaxy, with a tendency towards redder hues, indicative of an older stellar population. There is no morphological evidence of recent or ongoing major merger events, though subtle disturbances cannot be ruled out at this resolution. Based on its smooth appearance and color profile, it is likely an elliptical galaxy.