The galaxy presents as a relatively compact, though somewhat diffuse, object. A centrally concentrated bulge region is apparent, displaying a yellowish-orange hue indicative of an older stellar population. There are hints of a disk structure surrounding the bulge, but it appears quite faint and ill-defined. The disk, if present, does not exhibit clear spiral arm morphology. Overall, the galaxy's light distribution is somewhat smooth, suggesting either a relatively quiescent state or advanced stage of morphological transformation. However, there is a slight asymmetry to the galaxy shape, and a subtle distortion in the outer regions, possibly indicating a past or ongoing interaction or minor merger event. Any such interaction doesn't seem to be causing a strong burst of star formation, based on the overall color profile. The object's redshift indicates it's at a substantial cosmological distance.
