The galaxy presents as a moderately luminous, disk-dominated system, viewed at a high inclination. It exhibits a primarily smooth morphology with a slightly elongated, cigar-like shape. The central region appears brighter and more concentrated than the outer regions, with a color profile suggesting a somewhat older stellar population concentrated in the bulge. Faint indications of spiral arm structure are hinted at within the disk but are not sharply defined. There are only minor disturbances indicating either past or ongoing interactions with smaller galaxies. A possible slight warping of the disk may also indicate minor tidal interactions. Overall, the galaxy appears as a reasonably well-formed and relatively quiescent system.