The galaxy presents as a smooth, elongated structure. Its shape is decidedly cigar-shaped, with an apparent lack of spiral arm features or significant disk structure. The light distribution appears centrally concentrated, fading towards the edges. The core exhibits a reddish-orange hue, possibly indicating a population of older stars and/or significant dust obscuration. Moving outwards from the core, the galaxy takes on a slightly bluer tint, suggestive of some ongoing star formation, albeit at a low level. There is no clear evidence of any major ongoing mergers or tidal disturbances. Overall, the galaxy appears to be a relatively quiescent system.
