The galaxy presents an elliptical morphology, appearing largely smooth and featureless. Its core exhibits a bright, concentrated luminosity, suggesting a high stellar density and possibly the presence of an active galactic nucleus. The galaxy displays a color gradient, transitioning from a yellow/orange hue in the central region to a redder tint towards the outer edges. This color difference suggests an aging stellar population residing in the outer regions of the galaxy. There is minimal evidence of spiral arm structures or dust lanes, contributing to its overall smooth appearance. The galaxy shows some signs of minor tidal disturbances. It's estimated to be a relatively large galaxy with moderate star formation. The overall structure appears to be relatively undisturbed, with no signs of a major ongoing merger.
