The galaxy presents as a relatively compact and centrally concentrated object. It exhibits a smooth morphology, lacking any prominent spiral arms or distinct features suggestive of a disk structure. The overall shape appears approximately round but slightly oblong. There is no evidence of significant tidal disturbances, ongoing mergers, or major interactions with nearby galaxies. The galaxy's core displays a yellowish to orange color, possibly indicating an older stellar population or significant dust obscuration in the central region. Fainter, bluer light extends outwards, suggesting the presence of some younger stars or ongoing star formation, albeit at a low rate. The galaxy's overall luminosity is moderate. Its apparent size is small, indicative of its cosmological distance.
