The galaxy appears as a centrally concentrated object with a smooth, ellipsoidal morphology. There are no visible spiral arm structures. The galaxy exhibits a dominant yellowish core, suggesting an older stellar population. A redder, diffuse patch is observed on one side of the core, possibly indicating an area of active star formation or a dust lane. A fainter, bluer and more irregular object is present in close proximity, and may be interacting with the main galaxy or simply be in line of sight. This feature suggests the possibility of tidal disruption or a dwarf galaxy undergoing accretion. Overall, this galaxy could be classified as a massive galaxy that is undergoing either quiescence, or an interaction.
