The galaxy presents as an elliptical morphology, with a smooth, concentrated light profile. The central region exhibits a yellowish hue, potentially indicative of an older stellar population. Moving outward from the core, the galaxy displays a subtle color gradient, transitioning towards a slightly bluer periphery. This suggests the presence of a younger stellar population in the outer regions, albeit less pronounced than what is observed in actively star-forming spiral galaxies. There is no clear evidence of distinct spiral arms or prominent dust lanes. The galaxy appears relatively undisturbed, showing no signs of major mergers or tidal interactions. Faint wisps or irregularities can be seen extending from the main body of the galaxy, possibly remnants of minor interactions or ongoing accretion events. The overall roundness is indicative of a dynamically relaxed system.
