The galaxy presents as a largely smooth, centrally concentrated structure with a slight ellipticity. The light distribution suggests a dominant bulge component. There is a suggestion of faint extended emission surrounding the central region, contributing to a more diffuse appearance at the galaxy's periphery. The color profile indicates a generally blue hue, hinting at ongoing or recent star formation, although a central concentration appears somewhat brighter than the rest of the galaxy. There are no immediately obvious signs of strong tidal disturbances, major spiral arms, or a prominent disk structure based on the image. Overall, this appears to be a relatively undisturbed, intermediate-mass galaxy, possibly transitioning towards a more quiescent state.
