This galaxy presents as a smooth, elongated structure indicative of a disk galaxy viewed nearly edge-on. It exhibits a bright central bulge that appears yellowish-white in color, suggesting a population of older stars. A faint disk is observed extending outwards from the bulge, with hints of dust lanes or spiral arm structure visible on one side. The overall color of the disk is slightly bluer than the bulge, possibly indicating regions of more recent star formation, although this star formation appears subdued. There is no apparent sign of a major ongoing merger or significant tidal disruption. Faint irregularities on the disk could potentially be signs of minor disturbances, but these do not greatly affect the object's main shape. The galaxy appears to be relatively isolated, with no immediately apparent signs of interactions with other galaxies.
