The galaxy presents as an elliptical morphology, with a high degree of central concentration. It exhibits a smooth, featureless profile with no apparent spiral arms or distinct disk structure. The galaxy's color appears to be generally redder, possibly indicative of an older stellar population with diminished recent star formation. The overall shape is slightly elongated, although it is mostly round, without significant tidal distortions or signs of ongoing mergers. There is minimal evidence of dust lanes or prominent star-forming regions within the visible structure. The galaxy appears to be relatively isolated.
