The galaxy presents as a relatively smooth, elliptical morphology. It appears centrally concentrated, exhibiting a gradual radial falloff in luminosity. The core exhibits a yellowish-orange hue, suggestive of an older stellar population and potentially lower rates of ongoing star formation. Surrounding the core, a faint, more diffuse halo extends outwards, displaying a slightly bluer color profile compared to the core. There is no discernible spiral arm structure or prominent dust lanes visible, implying a classification towards early-type galaxies. The overall smooth appearance supports its classification as an elliptical galaxy with a substantial spheroidal component. There is no strong evidence for ongoing major mergers or significant tidal disturbances.
