The galaxy presents an overall elongated, cigar-shaped morphology. The central region exhibits a smooth, concentrated bulge, displaying a yellowish-orange hue, suggestive of an older stellar population. Moving outward from the bulge, the galaxy transitions to a disk-like structure, apparent from the side-on viewing angle. This disk component shows a greenish tint, possibly indicating the presence of ionized gas and ongoing star formation. There is some evidence of asymmetry in the outer regions, with one end exhibiting a slightly enhanced redness, potentially indicative of either a region of dust obscuration or a population of younger, redder stars. There is no obvious grand spiral structure, but subtle irregularities might be present. The galaxy appears relatively isolated, lacking any obvious signs of major tidal disturbances or a prominent interacting companion in its immediate vicinity.
