The galaxy presents as a single, somewhat rounded object with a smooth, featureless morphology. There appears to be no prominent spiral arm structure or central bar. There is evidence of a slight color gradient, with the central region appearing more luminous and slightly redder in hue, indicating an older stellar population and/or higher dust concentration toward the core. The outer regions appear bluer, suggesting the presence of younger, hotter stars. There is an area of minor disturbance visible, perhaps evidence of a small-scale interaction. The general roundness suggests that the galaxy may be closer to an elliptical type, or potentially a late-stage spiral that has undergone significant morphological transformation.
