The galaxy exhibits a morphology indicative of a system undergoing a merger. The primary body shows a smooth, somewhat elliptical profile, though the overall shape appears irregular. It appears to have an estimated effective radius in the range of approximately 7.5 kiloparsecs. The color of this component appears yellowish-orange. This suggests an older stellar population with a lower rate of star formation.

A second, smaller component is visible, connected to the primary body. This secondary structure displays a bluer color, indicative of more recent or ongoing star formation. Its morphology is less defined, further supporting the interaction hypothesis. There appears to be an interaction or tidal stream, indicative of advanced merger stage.

Overall, the galaxy appears to be a late-stage merger event, characterized by a combination of established stellar populations and regions of active star formation.
