The galaxy presents as a relatively compact object with a non-uniform distribution of light. There is evidence of both a smooth, centrally concentrated component and regions exhibiting more complex structure. A distinct, irregular feature extends from the central region, suggestive of a tidal tail or disrupted structure.

The galaxy displays a range of colors, with a dominant blue hue within the irregular extension, which indicates regions of active star formation. The central region appears more yellow, potentially due to an older stellar population or dust obscuration. The structure appears to be undergoing a merger or a strong interaction with another galaxy, as evidenced by the asymmetric light distribution and the irregular feature.
