The galaxy appears as a lenticular or early-type spiral, displaying a generally smooth, elliptical morphology. There is a bright, concentrated central bulge, gradually fading into the outer regions of the disk. The overall color suggests a population of older stars, although a subtle bluer hue in the outer disk indicates the possibility of some ongoing, low-level star formation. The galaxy appears relatively undisturbed, with no strong evidence of tidal features or ongoing mergers. There is a slight elongation, classifying it as not perfectly spherical, but not a highly flattened disk either. No distinct spiral arms are visible.
