The galaxy presents a morphology consistent with an elliptical galaxy. It exhibits a smooth, centrally concentrated luminosity profile with a high degree of radial symmetry. The isophotes appear generally elliptical with slight deviations. The core region displays the highest surface brightness, gradually decreasing outwards. There is a subtle color gradient, with the central regions appearing somewhat yellower than the outer regions, which have slightly redder hues. This may indicate a higher concentration of older stellar populations toward the galaxy's center. Faint asymmetry may indicate a possible tidal interaction or a minor merger event, though the galaxy is generally undisturbed. The overall structure suggests a dynamically relaxed system. The galaxy is relatively massive, exhibiting a red sequence population.
