The galaxy presents as a relatively compact object with an apparent radius of approximately 7.6 arcseconds. The central region exhibits a bright, concentrated core, surrounded by a fainter, diffuse halo. The overall color appears somewhat blue, potentially indicating the presence of younger stellar populations or active star formation within the central region. Evidence of significant disk structures is minimal from visual inspection alone.

There appears to be some possible merging activity occurring; there is minor visual disturbance.
