The galaxy presents as an elongated, cigar-shaped structure. It exhibits a smooth, relatively featureless morphology with a high degree of symmetry about its major axis. The central region displays a concentrated luminosity, appearing brighter and more orange-red in color, suggesting an older stellar population likely dominating the core. The outer regions gradually fade in intensity, with a subtle shift towards bluer hues. The color gradient from core to periphery may indicate ongoing star formation in the outer regions, although the smoothness suggests a generally quiescent star formation rate. No obvious spiral arms or distinct dust lanes are visible, which is further evidence this may be an elliptical type galaxy. There are no signs of significant tidal disturbances or ongoing mergers. The galaxy appears to be isolated and undisturbed.
