The galaxy presents as a reddish point source with an estimated effective radius of approximately 2 arcseconds. Morphologically, the object exhibits characteristics of both smooth and featured morphologies, with a slight preference towards a smooth appearance based on the data provided. However, there also appears to be some distortion or disturbance evident within the galaxy's structure, possibly indicating a minor interaction or merger event with another galaxy, though this is not as likely based on the data provided. A noticeable fraction of the light output is centered within a central concentration of stars. Overall, the image suggests a galaxy possibly undergoing a disturbance, without clear spiral arm structures.
