The galaxy presents as an elongated, cigar-shaped structure indicative of an elliptical morphology, viewed nearly edge-on. The central region exhibits a concentration of light, appearing yellowish-orange. Moving outward from the center, the luminosity gradually decreases, with the outer regions displaying a fainter, whitish hue. There is no readily discernible spiral arm structure or dust lane apparent in this image. The overall smoothness suggests the galaxy is a relatively evolved system, with a high fraction of older stellar populations concentrated in the bulge. There is some slight irregularity present on the edges of the disk, though, there doesn't appear to be evidence of a recent major merger.
