The galaxy presents a largely smooth, elliptical morphology with a high degree of central concentration. The light distribution appears relatively uniform, lacking any discernible spiral arms or prominent disk structures. It exhibits a mostly spherical shape but is slightly elongated. The galaxy's color profile indicates a redder hue, suggesting a population dominated by older stars and relatively low current star formation activity. No signs of major mergers or tidal disturbances are readily apparent. The galaxy exhibits a central core that appears especially bright. There are no apparent signs of active galactic nuclei activity, although further spectroscopic data would be needed for confirmation. Overall, the galaxy appears to be an evolved system consistent with an elliptical classification.
