The galaxy presents as a centrally concentrated object with a generally elliptical morphology. There appears to be a bright, yellowish core, potentially indicative of an older stellar population and/or a central supermassive black hole. The surrounding disk exhibits a bluer hue, suggesting ongoing star formation. The structure is not entirely smooth; there are hints of subtle disturbances or faint spiral arm-like features extending outward from the central region, though these are not sharply defined. The outer regions of the galaxy appear somewhat diffuse and irregular, lending to a more amorphous overall shape. No major tidal features or signs of a major merger are immediately apparent. The overall impression is that of a galaxy undergoing some level of evolutionary activity, possibly minor interactions or internal processes driving star formation.
