The galaxy exhibits a roughly elliptical morphology, with a slight elongation that deviates minimally from a circular shape. A central bulge region is visible, displaying a yellowish-white hue, suggesting a population of older stars. Surrounding the bulge is a fainter, more diffuse disk component. This disk shows hints of blue coloration, indicative of ongoing star formation. There is a weak suggestion of some disrupted structure that appears to be a tidal arm on one edge, but for the most part the structure is consistent with a non-interacting galaxy.

Based on these properties, this galaxy is likely a spiral galaxy undergoing active star formation in its disk, but approaching a transition towards a morphology where the disk will become much more diminished. It is possible that it has had a minor merger recently that caused some weak tidal features to become visible.
