The galaxy presents as a moderately bright, centrally concentrated object. Its light profile appears relatively smooth, with a subtle elongation that suggests a shape somewhere between spherical and disk-like. There is a lack of prominent spiral arm structure or a well-defined bulge; the light fades gradually outwards from the center. The color is somewhat redder than that of typical spiral galaxies, pointing to an older stellar population, but there appears to be some blue color, suggesting a low level of ongoing star formation. No significant signs of major mergers or tidal disturbances are apparent. There are very minor disturbances and low disk features.
