The galaxy presents as a centrally concentrated, smooth object. Its light is dominated by a yellowish-white hue at the core, suggesting an older stellar population. The outer regions exhibit a subtle bluish tint, indicative of some younger, hotter stars, though the overall star formation rate appears relatively low. The galaxy's morphology appears close to elliptical, with a high degree of radial symmetry. There are no obvious signs of spiral arms or a distinct disk structure. Subtle distortions may be present in the outer envelope, hinting at a possible past interaction or minor merger event, although it is generally undisturbed. The galaxy's size seems moderate, appropriate for a mid-mass system.
