The galaxy presents as a largely smooth, elliptical-like structure with a concentrated central bulge. Its color profile leans towards the redder end of the spectrum. There is an adjacent, smaller object in close proximity. This secondary object appears less red, potentially indicating a difference in stellar population or dust content compared to the primary galaxy. The galaxy's overall form suggests a relatively evolved system, possibly with a cessation of significant star formation activity, though the presence of the adjacent object may suggest an ongoing or past interaction.
