The galaxy appears as a single, moderately concentrated object with a centrally brightened core. There appears to be some asymmetry present within the central region. A diffuse stellar halo surrounds the core, with irregular extensions which may be signs of tidal interactions or mergers with other galactic bodies. The object displays a relatively smooth overall morphology, but there are some subtle features suggestive of internal structure or disturbances. The primary coloration is yellowish-orange, possibly indicating an older stellar population. Subtle blue regions are observable in the periphery of the object, indicating the presence of ongoing star formation, albeit at a low level. Overall, the galaxy shows an intermediate level of evolutionary development, possibly transitioning from a more active star-forming phase to a more quiescent state.
