The galaxy presents a centrally concentrated morphology, appearing largely smooth and elliptical. There is a slight elongation, but it is generally round in appearance. The core exhibits a bright, yellowish hue, suggesting a population of older stars. The outer regions fade gradually into the background, with subtle hints of redder tones, possibly indicating areas of dust obscuration or older stellar populations at the periphery. There's no clear evidence of spiral arms or prominent disk features. Overall, the galaxy seems relatively undisturbed, without strong signs of ongoing mergers or tidal interactions.
