This galaxy exhibits an elliptical morphology, presenting as a smooth, centrally concentrated distribution of light. The central region displays a yellow-orange hue, suggestive of an older stellar population and minimal ongoing star formation. The galaxy is elongated, deviating from a perfectly circular shape, with an approximate major axis of 7.6 kpc. Faint, diffuse blue light can be detected in the outer regions of the galaxy. There is no strong evidence of spiral arm structure or active star-forming regions. The overall appearance indicates a relatively evolved galaxy with a significant stellar mass. No signs of major mergers, only hints of minor disturbances present.
