The galaxy presents an elliptical morphology, exhibiting a high degree of central concentration. The light profile appears smooth, with no readily discernible spiral arms or bar structures. The color gradient suggests a relatively old stellar population, with a yellowish-white core possibly indicative of a bulge dominated by evolved stars. There appears to be a faint bluish hue extending outwards from the core, possibly suggesting the presence of some younger stars or ongoing low-level star formation in the outer regions. No significant signs of tidal disturbances or major mergers are visually apparent. The galaxy appears undisturbed and exhibits a regular morphology.
