The object presents as a relatively compact galaxy with a moderately elliptical morphology. It shows a complex internal structure exhibiting characteristics suggestive of a disturbed system. Notably, there appears to be a faint tidal tail or stream extending from the main galactic body, indicating possible past or ongoing gravitational interaction with another object. The galaxy's color is predominantly reddish, implying an older stellar population and potentially significant dust obscuration. There is little evidence of prominent spiral arms or distinct features within the disk, lending further support to the possibility of a more spheroidal, bulge-dominated galaxy. The observed features may be indicative of a recent or ongoing merger event, causing the observed irregularities in its overall structure. High levels of disturbance coupled with little presence of spiral arms suggest a recent major disturbance. 
