The galaxy appears as a relatively small, face-on or nearly face-on spiral. It exhibits a central bulge with a slightly elongated shape. The spiral arms are not very well-defined, giving the galaxy a somewhat diffuse appearance. There are hints of dust lanes within the arms. The color suggests a mix of stellar populations, with some bluer regions indicative of recent star formation and redder regions suggestive of older stars. The galaxy's overall morphology leans toward being relatively smooth, but with subtle features, and is moderately rounded. There are indications of a possible minor disturbance or interaction, perhaps an ongoing merger event. The galaxy's luminosity suggests it is of considerable size and mass.
