The galaxy presents a largely smooth, elliptical morphology with a concentrated central bulge that appears luminous. It exhibits a gradual decrease in luminosity from its core outwards, characteristic of early-type galaxies. There is a slight elongation along one axis, deviating minimally from a perfectly circular form. No distinct spiral arms or prominent dust lanes are apparent. The color profile suggests a relatively homogeneous stellar population, consistent with older stars. There may be minimal ongoing star formation. There is no indication of any significant tidal disturbances or recent merger events.
