The galaxy presents as a relatively smooth and rounded structure. It lacks any visually prominent spiral arms or a well-defined disk. The central region exhibits a higher concentration of luminosity, suggesting a bulge component. A color gradient is observable, with the core appearing more reddish-orange, potentially indicating an older stellar population or dust obscuration. The outer regions appear bluer in color, which could indicate the presence of some younger, hotter stars, but it's not as well-defined or prominent as one would expect to see in a normal spiral galaxy. There is no strong evidence of any major ongoing merger or significant tidal disturbances based on the overall morphology, but some minor asymmetry cannot be entirely ruled out. Overall, the galaxy exhibits characteristics consistent with an elliptical galaxy.
