The galaxy appears as a relatively compact object, exhibiting a moderate level of internal structure. The light distribution suggests a morphology somewhere between smooth and exhibiting spiral features. It presents a disk-like appearance without well-defined spiral arms. The colors indicate a range of stellar populations, with a tendency towards redder hues, possibly indicating an older stellar population. There appears to be some ongoing star formation activity. The shape is moderately elliptical, not quite spherical but not highly elongated either. There are no strong indications of any major ongoing merger events, though some minor disturbances may be present in the form of subtle asymmetries or tidal features. Overall, the galaxy appears to be a disk galaxy that is undergoing a period of moderate evolution.
