The galaxy presents an elongated, cigar-shaped morphology. It appears to be generally smooth in texture with a concentrated central bulge that is brighter than the surrounding galactic disk. The galaxy's light profile transitions gradually from the center outwards, with no obvious distinct structures or spiral arm features visible in this observation. There is a subtle color gradient visible, with the central region exhibiting a more yellow to white hue, suggestive of an older stellar population, while the outer regions show a slightly bluer tint, possibly indicating the presence of younger stars or ongoing star formation at a low rate. There does not appear to be evidence of any major ongoing merger activity or significant tidal disturbances affecting the galaxy's structure. The galaxy appears generally undisturbed, though the possibility of a very minor interaction cannot be fully excluded based on this image alone.
