The galaxy appears as a centrally concentrated object with a smooth, diffuse light profile, indicative of a spheroid-dominated morphology. There is a notable lack of spiral arm structure or prominent dust lanes visible in this image. The object exhibits a color gradient, transitioning from a more bluish hue in the outer regions to a reddish or pinkish hue towards the central region, potentially suggesting a higher concentration of older stellar populations, and therefore less star formation, within the core, while the outer areas contain a younger population of stars. No obvious signs of tidal disturbances or ongoing mergers are detected within the immediate vicinity of the object. The light distribution appears mostly symmetrical.
