This galaxy presents as a slightly elongated object, with an observed blue hue indicating the presence of younger stellar populations and ongoing star formation. The morphology appears somewhat disturbed, potentially suggesting recent or ongoing gravitational interactions with other galaxies or internal dynamical processes. The light distribution is not uniformly smooth, and possibly shows internal structures. There is evidence of clumpy regions of active star formation. The galaxy appears to be undergoing a minor merger and is cigar shaped.
