The galaxy presents as a relatively smooth object, with a noticeable lack of defined spiral arms or prominent features. The overall shape is somewhat elliptical, displaying a slight elongation. Color gradients suggest an older stellar population, concentrated in the central bulge, which displays an orange hue. A surrounding, fainter disk-like component is visible with a greenish tint. This color may indicate recent or ongoing star formation. There is no obvious indication of a major merger or significant tidal disruption. There is no prominent dust lane visible.
