The galaxy presents as a relatively smooth, elongated structure. Its central region appears brighter and more yellow-white in color, suggesting an older stellar population. The outer regions exhibit a bluer hue, possibly indicating younger stars or ongoing star formation. The galaxy's elongated shape is more cigar shaped than circular, indicating that it is not a spiral galaxy, but an elliptical galaxy. There appears to be some minor tidal distortion present, but the system does not indicate signs of any major interactions or mergers. The galaxy does not show any strong dust lanes or prominent spiral arm features within its disk, nor do there appear to be any active galactic nuclei present.
