The galaxy appears as a relatively compact object, approximately 6.6 kpc in radius. It exhibits a primarily smooth morphology, with a slightly fuzzy appearance and little to no immediately discernable spiral structure. The color profile indicates a redder hue, suggesting an older stellar population and a low rate of star formation. There is a subtle central concentration of light, which could indicate a bulge or an active galactic nucleus, though this is uncertain based on the image alone. The overall smooth texture and color suggests it is likely an elliptical or lenticular galaxy. There is no evidence of a major ongoing merger, though some minor tidal disturbances may be present.
