The galaxy presents an overall smooth morphology, appearing largely spheroidal in shape, although not perfectly circular.  It exhibits a centrally concentrated luminosity profile, with a bright core that gradually fades outwards. There is a hint of a more disc-like structure or feature to the right, possibly an ongoing minor interaction that is causing some morphological disturbance. The primary body of the galaxy displays a bluish hue, suggestive of some ongoing star formation. There's a secondary, adjacent region that appears less defined and redder in color, potentially indicative of an area with an older stellar population, higher dust content, or the result of a galaxy merger. Overall, the galaxy does not appear to be strongly disturbed, though some level of gravitational interaction cannot be ruled out.
