The galaxy presents a generally smooth and rounded morphology. It appears as a single, somewhat diffuse, object with a relatively homogeneous light distribution. There is a subtle color gradient visible, hinting that the central region may exhibit slightly redder hues compared to the outer areas. No distinct spiral arms or bar structures are discernible; the overall form is reminiscent of an elliptical galaxy, or perhaps a lenticular galaxy viewed at a sufficient distance that finer details are blurred. There is no obvious evidence of significant ongoing star formation in the visible light spectrum. Any potential tidal features or signs of recent mergers are subtle or absent; the galaxy appears to be relatively undisturbed in its present state. The object exhibits a moderate degree of compactness.
