The galaxy presents as a relatively smooth, elongated object with a high degree of central concentration. It exhibits a cigar-like shape. The primary color is a faint bluish-white, suggesting the presence of at least some young, hot stars or potentially an active galactic nucleus. There are some faint hints of what may be spiral arm structure or dust lanes, but they are not well-defined, with much of the light being concentrated at the center. There is no indication of any major mergers or significant tidal disturbances. The overall morphology points towards an early-type spiral or lenticular galaxy, possibly with ongoing, though not vigorous, star formation.
