The galaxy appears as a centrally concentrated object, exhibiting an overall elliptical morphology. Its core is relatively bright and displays a yellowish-red hue, potentially indicating a population of older stars or significant dust obscuration. The outer regions of the galaxy appear more diffuse and exhibit a faint blueish-green color, suggesting the presence of some younger stellar populations or ongoing, albeit limited, star formation. The galaxy's structure is largely smooth, with no apparent spiral arms or significant disturbances visible. It appears to be a relatively isolated system, showing no signs of major mergers or tidal interactions with other galaxies in its immediate vicinity. A slight elongation is observed, giving it a shape between a perfect circle and a more elongated cigar shape.
