The galaxy presents a distinct, elongated morphology, resembling a cigar shape. The light distribution is concentrated towards the center, displaying a bright, diffuse core indicative of a central bulge. The disk appears relatively smooth and featureless, lacking prominent spiral arm structures. The color profile shifts from a slightly yellower hue in the core to a bluer tint in the outer regions of the disk, suggesting the potential for some star formation activity away from the bulge, yet not pronounced. The galaxy shows a strong central concentration with a hint of a disk, typical of an intermediate-type spiral or lenticular galaxy. There's no visual evidence of significant ongoing mergers or major tidal disturbances. The overall appearance is that of a moderately massive galaxy at a considerable distance, with a relatively quiescent disk.
