The galaxy presents as a lenticular or possibly a spiral galaxy viewed at a high inclination angle, close to edge-on. The light is centrally concentrated with a smooth profile. The overall shape is elongated and appears cigar-shaped. There's some evidence of a faint, diffuse disk. The colors appear bluer towards the center of the galaxy, possibly indicating a population of younger stars. The outer regions are dimmer and have a redder hue, possibly indicating older stellar populations and dust obscuration. There is no visible evidence of strong spiral arms, active star formation regions, or interactions with other galaxies. The morphology suggests it may be relatively undisturbed.
