The galaxy presents an elliptical morphology. It exhibits a smooth, centrally concentrated light distribution, suggestive of an older stellar population. The core region displays a bright yellowish-orange hue, potentially indicating a higher density of evolved stars and dust. The outer regions fade gradually into the background, displaying a more diffuse and redder coloration, perhaps due to a lower density of stars and the presence of older stellar populations. There is no clear evidence of spiral arms or prominent dust lanes. The galaxy appears relatively undisturbed, showing no major signs of recent merger activity or tidal interactions. Overall, the galaxy seems to be a relatively massive system, currently undergoing low levels of star formation.
