The galaxy presents an elongated, cigar-shaped morphology. It appears relatively smooth in texture, lacking any immediately obvious spiral arms or distinct features such as dust lanes. The light distribution is centrally concentrated, with a gradual decrease in intensity towards the outer regions. The color profile suggests a predominantly older stellar population, as indicated by the reddish hue, although there is evidence of some bluer regions, particularly in the central area, potentially indicative of ongoing, albeit relatively low-level, star formation. No signs of major mergers or significant tidal disturbances are visible; however, a minor disturbance cannot be ruled out based solely on the available imagery. The overall structure suggests a galaxy that is either elliptical or a smooth disk galaxy viewed edge-on.
