The galaxy presents a moderately luminous profile with an estimated redshift indicating a considerable distance. It exhibits an overall elliptical shape with some deviation toward a disk-like structure. The central bulge is prominent and appears relatively smooth and concentrated, displaying a yellowish-white hue, suggesting an older stellar population. The outer regions show a faint bluish tint, possibly indicative of ongoing or recent star formation, though the rate appears moderate. There is a subtle irregularity or disturbance detectable in the morphology of the galaxy suggesting minor interactions or internal dynamics affecting its structure. There are no obvious signs of a major merger event such as tidal tails. Overall, the galaxy appears as a transitionary object, displaying characteristics of both elliptical and spiral galaxies, potentially in the later stages of its evolution.
