The galaxy appears to be a spiral galaxy, though viewed at an angle that makes it difficult to assess arm structure. There is evidence of some patchy, asymmetric light distribution. The galaxy does not appear to have a strong central bulge, and the disk component is dominant. There is no evidence of a major merger or significant tidal disruption. The galaxy has an estimated mass of 10^10 solar masses, with the estimated star formation rate (SFR) being relatively quiescent. Overall, the object appears to be a relatively isolated spiral galaxy with limited ongoing star formation.
