The galaxy presents as a smooth, elliptical object with a high degree of central concentration. Its overall shape is moderately elongated, appearing somewhat cigar-shaped, with a gradual decrease in luminosity from the core outwards. The central region exhibits a yellowish-white hue, indicative of an older stellar population. Fainter, bluer light is detectable in the outer regions, suggesting some ongoing, though likely limited, star formation. There is no clear evidence of spiral arms or a well-defined disk structure, instead, the light is diffusely spread across the galaxy's body. No significant signs of tidal disruption or interaction with other galaxies are apparent. The galaxy appears relatively undisturbed, exhibiting a primarily elliptical morphology.
