The galaxy presents as a centrally concentrated object with a generally smooth morphology. The core exhibits a bright, possibly unresolved, emission. There is evidence of a surrounding, fainter halo, though its structure is not well defined. The overall color appears to be skewed toward the redder end of the spectrum, suggesting an older stellar population or significant dust obscuration. The object lacks any prominent spiral arms or other distinct features typically associated with actively star-forming galaxies. There are a few nearby objects that may be associated with the galaxy, such as a faint source to the upper right which may be a minor disturbance within the galaxy. This object is likely a massive galaxy, on the order of 10^11 solar masses.
