The galaxy appears to be a relatively compact object with a discernible central bulge that is the brightest region in the image. The overall shape is somewhat elliptical, but exhibits some irregularities. There is faint evidence of a disk-like structure surrounding the bulge, but the low surface brightness of the surrounding light makes a definitive classification difficult. The color gradient suggests a stellar population gradient, with bluer colors concentrated towards the edges, potentially indicative of younger stars in a more active star forming region. I would classify this galaxy as likely not merging, but possibly having experienced a minor disturbance based on the asymmetry and overall appearance. It doesn't appear to be a pure elliptical, nor a spiral, so it may be an irregular type galaxy. There is no strong indication of tidal tails or other features usually associated with major mergers.
