The galaxy presents as a moderately bright, elliptical-shaped structure. Its core exhibits a concentrated luminosity, appearing nearly spherical. This central region transitions smoothly into a more diffuse outer halo. The overall color profile suggests a relatively evolved stellar population, as the core leans towards yellow-red hues. The disk component is not clearly visible, but it appears to be present. The outer regions of the galaxy have bluer hues than the inner regions. The galaxy appears largely undisturbed, without strong tidal features or obvious signs of a major merger event. Faint spiral arms are visible.
