The galaxy presents as an elliptical morphology, with a relatively smooth light distribution and high central concentration. The color profile is dominated by yellow-red hues. The light suggests an older stellar population, with likely little to no active star formation. The galaxy exhibits a slight deviation from perfect roundness. There is some indication of a minor disturbance, possibly due to a past interaction, but no strong evidence of a major merger or tidal features. The galaxy appears as an isolated object in this field of view.
