The galaxy presents as a relatively compact and centrally concentrated object. The light profile appears smooth and elliptical in nature, lacking any distinct spiral arm structure or prominent dust lanes. The core exhibits a brighter, more intense glow, suggesting a higher density of stars and potentially an active galactic nucleus. Overall, the galaxy's morphology appears to be relatively undisturbed, showing no obvious signs of major mergers or tidal interactions with other galaxies. The color index is relatively red, implying an older stellar population with a lower rate of on-going star formation. The estimated effective radius suggests a moderate physical size. 
