The galaxy presents an elongated, cigar-shaped morphology. It is a relatively bright object with a smooth appearance, but with some possible features. The central region is characterized by a yellowish hue, potentially indicating an older stellar population. The outer regions exhibit a bluer tint, suggesting the presence of younger, hotter stars and the potential for ongoing or recent star formation. There appears to be no major merging event occurring, and only some possible minor disturbance. The redshift indicates the galaxy is relatively distant and being observed as it was in the past. The estimated mass is large, which supports the mature appearance of this galaxy.
