The galaxy presents a largely smooth and rounded morphology, suggestive of an elliptical type. Its core exhibits a concentrated, bright yellowish hue, indicative of an older stellar population. Moving outward from the center, the light gradually diminishes, transitioning to a bluer halo. This may represent a smaller population of younger, hotter stars. There is no clear evidence of spiral arms or a distinct disk structure. The galaxy appears largely undisturbed, showing no signs of major mergers or tidal interactions, though a slight asymmetry cannot be ruled out with this image. The light appears mostly uniform and without distinctive knots or features. Based on its apparent size and color, it is likely a moderately massive system. The inferred star formation rate is relatively low.
