The galaxy presents as a luminous, centrally concentrated object with a somewhat smooth morphology. The central region exhibits a yellowish-white hue, suggesting a population of older stars. Moving outwards from the core, there is a subtle transition into regions with a bluish tint, especially at the edges and towards the bottom half of the disk. These bluer regions imply the presence of younger, hotter stars and possibly ongoing star formation activity. The galaxy appears to be slightly elongated, tending toward a flattened, disc-like structure with a very slight disturbance. There are hints of possible tidal disturbances in the lower portion of the galaxy. The overall structure indicates it is transitioning between a spiral and elliptical galaxy, displaying a more complex and dynamic environment than a standard elliptical.
