The galaxy presents as a relatively small, elongated structure, appearing cigar-shaped. Its morphology suggests a possible edge-on spiral or an elliptical galaxy with a pronounced asymmetry. The central region exhibits a brighter concentration of light, possibly indicative of a galactic bulge. The light from the galaxy appears bluer than the light surrounding it. There is no evidence of any major merging activity or strong tidal features, although a minor disturbance cannot be entirely ruled out.
