The galaxy presents as a somewhat elliptical structure with a bright, concentrated central bulge. The core exhibits a yellowish-white hue, suggestive of an older stellar population. Moving outward from the core, the galaxy displays a fainter, more diffuse halo. There is evidence of a disk component, albeit not sharply defined. Faint bluish tinges can be observed in the outer regions of the disk, hinting at the presence of younger, hotter stars and possible ongoing star formation. The overall appearance is relatively smooth, with no prominent spiral arms or significant dust lanes visible in this image, which would make this likely an early type galaxy. There are subtle irregularities in the outer halo, which might be evidence of past merger events or interactions. The galaxy exhibits a measurable redshift, placing it at a considerable cosmological distance. Its apparent size corresponds to a moderate physical diameter.