The galaxy presents as a predominantly smooth, elliptical morphology. The central bulge exhibits a concentrated, bright luminosity. Moving outwards from the core, the intensity of light decreases gradually towards the periphery, where the boundary becomes somewhat indistinct. Faint hints of a disk component are possibly present but are not well-defined. There is no clear indication of spiral arms or bar structure. The overall shape is close to round, displaying only a slight elongation. There is some evidence of minor tidal disturbance or ongoing interaction, but no indications of major merging activity. The color profile exhibits a tendency towards redder wavelengths.