The galaxy presents as a relatively smooth, elliptical-like structure. Its central region exhibits a concentrated luminosity, appearing a warm, golden hue. This intense core gradually fades outwards into a more diffuse halo. There is no prominent disk-like structure immediately apparent, nor any distinct spiral arm features. The galaxy is moderately round in overall shape, though subtle irregularities in the outer regions suggest possible minor tidal disturbances or interactions. Overall color appears largely homogeneous across the galaxy, with subtle variations in the outskirts that could indicate regions of ongoing, although limited, star formation. The light distribution appears largely centrally concentrated.
