This galaxy presents a predominantly smooth, elongated morphology. The overall color is a yellow-white hue, suggesting a population of older stars. A slight color gradient is visible, with the central region appearing more yellow and the outer regions exhibiting a bluer tint. This could indicate ongoing, though perhaps limited, star formation in the galaxy's periphery, possibly due to past minor disturbances that haven't completely disrupted the overall smooth structure. The galaxy appears relatively undisturbed, with no signs of major mergers or tidal features. The axial ratio suggests an elliptical or lenticular classification, viewed at a significant angle. 
