The galaxy presents as an elongated, cigar-shaped structure. A central bulge is present, exhibiting a smooth, diffuse light profile that transitions into a fainter disk component. There is a subtle color gradient visible across the galaxy, transitioning from a generally pale yellow hue in the central bulge to a bluer tint towards the outer edges of the disk. This suggests a potential difference in stellar populations, with the central bulge potentially dominated by older stars and the disk containing regions of more recent star formation. The galaxy appears relatively undisturbed, with no obvious signs of major merging activity. The system does not have any particularly pronounced spiral arm structure. There may be some very faint, diffuse structures extending from the disk, potentially tidal features, although it is difficult to confirm.
