The galaxy presents a largely smooth morphology, with a dominant spheroidal component. It appears elliptical in shape, exhibiting a high degree of radial symmetry. The galaxy's color profile suggests an evolved stellar population, with a predominantly red-yellow hue across its body and with no visible dust lanes. This observation is consistent with a lack of significant ongoing star formation, though some low level cannot be excluded. The galaxy displays no obvious signs of spiral arms or a central bar structure. There are also no indications of tidal features, major disturbances, or ongoing merger activity in this image. The light appears relatively concentrated towards the core.
