The galaxy presents as a largely featureless elliptical or lenticular morphology, with a high degree of central concentration. The light profile is smooth and well-defined, displaying a near-spherical shape with some deviation towards a slightly elongated form. The galaxy exhibits a distinct color gradient, transitioning from a yellowish-orange core to a redder outer halo. This suggests a stellar population dominated by older, redder stars. The lack of discernible spiral arms or dust lanes indicates a relatively quiescent galaxy, with minimal ongoing star formation. There is no evidence of any major mergers or tidal disturbances in the immediate vicinity. The overall impression is of a massive, evolved galaxy with a stable structure.
