The galaxy presents as an elongated, cigar-shaped structure, exhibiting a concentrated central bulge that appears yellowish-white in color. The luminosity is brighter towards the center, suggesting a higher stellar density in the galactic nucleus. Extending outwards from the central bulge, a diffuse disk component is visible, fading into the background. This disk appears less structured, without clear spiral arm features. The overall color gradient shifts from the yellowish-white core to a slightly bluer hue in the outer regions of the disk. There is a hint of a minor disturbance, either a slight asymmetry or a faint tidal feature on one edge of the disk, and it is unknown if this is due to a minor merger.
