The galaxy presents as a relatively smooth, elliptical structure. Its overall shape is elongated, leaning towards a cigar-like appearance, with no discernible spiral arms or bar features. A bright, concentrated central bulge dominates the galaxy's morphology, exhibiting a yellowish-white hue. Moving outward from the core, the galaxy's color transitions into a bluer, less intensely colored halo. There is some evidence of minor disturbances in the surrounding area but no clear signs of an ongoing major merger or significant tidal interactions. The smooth appearance of the galaxy suggests it has largely completed the merging process or that it has been quiescent for a considerable period. Its moderate redshift indicates that we are observing this galaxy at a significant cosmological distance. The limited presence of strong star formation regions implies that the galaxy's stellar population may be dominated by older stars.
