The galaxy presents as a relatively smooth, elongated structure. It exhibits a somewhat cigar-like shape, with a high aspect ratio. The central region appears brighter and more concentrated, suggesting a possible bulge. There is a color gradient from the center outwards, shifting from reddish hues in the core towards more greenish-blue tones in the outer regions. The galaxy displays no obvious spiral arm structures or significant dust lanes. There are no major indications of tidal disturbances or ongoing mergers. The galaxy appears to be a relatively undisturbed, lenticular or elliptical type system.
