The galaxy presents as an elongated, cigar-shaped structure. It appears to be relatively smooth, lacking significant distinct features like prominent spiral arms or strong dust lanes. The central region exhibits a concentrated, yellowish-white hue suggesting a higher density of older stars, possibly an aging stellar population within a bulge. Progressing outwards from the center, the color shifts to a slightly bluer tint, indicating the presence of younger stars in the galactic disk. There is a subtle asymmetry to the outer edges of the galaxy, suggesting a possible interaction or past merger event. No tidal tails or other clear indicators of active merging are evident. The overall morphology is indicative of a disk galaxy, likely viewed at a high inclination.
