The object presents as a relatively small, disk-shaped galaxy, observed at a high inclination angle, possibly close to edge-on. The central bulge is prominent, appearing bright and relatively smooth, with a concentrated light profile. There appears to be some evidence of a dusty disk surrounding the bulge, which may be obscuring some light from the center. The dust lanes appear patchy and are mainly along the plane of the disk. The outer regions of the disk show a red hue and may possibly be disrupted. There is a slight suggestion of tidal distortions. Based on morphology, this could possibly be a spiral or lenticular galaxy undergoing a minor merger. Further investigation of spectral data is warranted to confirm the nature of the galaxy and the possible presence of merger activity.
