The galaxy presents as a relatively faint, elongated object. Its overall shape appears to be a prolate spheroid. A bright, concentrated central bulge is observed, exhibiting a smooth and somewhat amorphous structure. Extending outward from the bulge, the galaxy appears to have a diffuse, flattened disk. The disk component shows hints of structure, although detailed features are difficult to resolve. The disk appears bluer in color relative to the central bulge, suggesting the presence of younger stellar populations and ongoing star formation. There is no visual evidence of a recent major merger, although subtle distortions or minor tidal features cannot be ruled out based on this image alone. The galaxy displays a red-shift, suggesting it is relatively distant.
