The galaxy presents an elliptical morphology, exhibiting a smooth, diffuse light profile with a high degree of roundness. Its core region shows a distinct, concentrated glow, suggesting a dense stellar population. The galaxy appears to be a mature system, potentially exhibiting a paucity of ongoing star formation. A fainter, more amorphous structure is observed in close proximity, suggesting a possible galactic interaction or the presence of a dwarf galaxy in the process of being tidally disrupted. The system as a whole does not display strong signs of major merging activity, instead suggesting that the faint structure may be either a companion galaxy or a tidal feature of a past interaction.
