The galaxy appears as a slightly elongated, diffuse object. The central region exhibits a relatively smooth morphology. There are some subtle disturbances in the galaxy's form, possibly indicating minor tidal interactions or internal instabilities. A portion of the galaxy exhibits a pronounced blue hue, potentially indicative of recent star formation activity. Additionally, the galaxy displays evidence of a redder component, likely representing an older stellar population or dust obscuration. There is a possible merger nearby, though there is no other obvious indications of a spiral disk galaxy. It would be beneficial to look at this object more closely to confirm whether it is an elliptical or lenticular galaxy, or a merging system. 
