The galaxy presents as a centrally concentrated object with a generally smooth, elliptical morphology. The core is intensely luminous, appearing nearly uniform in color, with a yellow-white hue, indicating an older stellar population. The overall shape is roughly circular, with a slight elongation. There is very little evidence of spiral arm structures or prominent dust lanes. A subtle color gradient is detectable, with the central region exhibiting a slightly warmer color temperature than the outer halo, which appears more diffuse. There is no indication of any major mergers or significant tidal disturbances.
