This galaxy presents as a smooth, centrally concentrated object. The light profile appears relatively featureless, suggesting an elliptical morphology or a lenticular galaxy viewed face-on. The color distribution is slightly redder in the central region, becoming slightly bluer toward the outer edges. This may indicate an older stellar population concentrated towards the center with a hint of ongoing star formation in the outskirts. There is no obvious evidence of spiral arms, bars, or significant dust lanes. The galaxy exhibits a round shape, lacking any significant elongation or tidal disturbances. This is consistent with it being a relaxed system that is unlikely to be undergoing a major merger or interaction.
