The galaxy appears as a centrally concentrated, luminous object with a fairly smooth morphology. There is little evidence of distinct spiral arms or a prominent disk structure. The object appears to have an elliptical shape, with a moderate ellipticity. The central region exhibits a bright, yellowish color, potentially indicative of an older stellar population. The outer regions appear fainter with a slight blueish hue, which could suggest the presence of some younger stars or ongoing, but low, levels of star formation. Overall, the galaxy presents a well-defined structure, with no obvious signs of major mergers or significant tidal disturbances.
