The galaxy appears as a centrally concentrated object with a smooth, elliptical morphology. The core exhibits a bright, yellow-white glow, suggesting a significant population of older stars. The overall shape is elongated, displaying a cigar-like structure, but it is still relatively smooth and featureless. There is minimal evidence of distinct spiral arms or active star formation regions. A faint halo extends outwards from the central region, gradually fading into the background sky. There are no obvious signs of any recent or ongoing merger activity or tidal disturbances, implying the galaxy is relatively undisturbed.
