The galaxy presents a largely smooth, cigar-shaped morphology. There is a noticeable lack of distinct spiral arms or a well-defined disk structure. The light is concentrated towards the center, suggesting a bulge, with the color indicating an older stellar population, with few sites of active star formation. Faint, diffuse extensions are present at either end of the major axis, possibly tidal tails indicative of past minor interactions or mergers, though a single merger seems unlikely. Overall, the galaxy exhibits characteristics consistent with a relatively evolved system, potentially an elliptical or lenticular galaxy at redshift z=0.121. The presence of even slight disturbances in the morphology is consistent with ongoing or recent interactions.
