The galaxy presents as a somewhat amorphous structure with a dominant central bulge. This bulge exhibits a yellowish-white hue, suggestive of an older stellar population. Extending from the main body is a fainter, bluish arm or tidal tail. The bluish coloration hints at ongoing star formation within this region. There is a slightly distorted morphology within the main body, implying past or ongoing interactions that may be causing some merger disturbances. The galaxy itself appears moderately luminous, with a notable color gradient moving from the bulge towards the outer arm. Overall, it appears to be an intermediate mass galaxy, possibly a spiral undergoing some kind of merger or tidal event.
