The galaxy presents as a somewhat elliptical, smooth structure with a concentrated central bulge. It appears to be relatively isolated and undisturbed, showing no signs of tidal tails or significant distortions indicative of recent major merger activity. The color gradient suggests an older stellar population dominating the central region, exhibiting a yellow-orange hue, while the outer regions display a bluer tint. This implies ongoing, though perhaps subdued, star formation in the galaxy's outskirts. The overall morphology indicates a system that is either an elliptical galaxy or a spiral galaxy transitioning to a lenticular type. The axial ratio is close to one, suggesting it is not highly inclined to our line of sight. There might be some minor asymmetry or irregularity in the outer regions of the galaxy, although the overall smoothness and lack of major disturbances suggest these are not significant.
