The galaxy presents an elliptical morphology, appearing largely smooth with minimal discernible substructure. It exhibits a high degree of central concentration, with a bright, well-defined nucleus. The light profile appears to diminish gradually outward from the core, suggesting a relatively old stellar population. The major axis of the galaxy is visibly longer than its minor axis, indicating an elongated shape, although it appears generally rounded. There is no evidence of strong tidal features, merging activity, or significant dust lanes. Color gradients suggest a redder core and slightly bluer outer regions, possibly indicating ongoing star formation in the disk, however the overall star formation activity is low. There is no visual evidence to suggest it is undergoing any significant interaction.
