The galaxy presents an elongated, somewhat irregular morphology, appearing cigar-shaped. There is evidence of a smooth central bulge region from which the light appears most intense. The galaxy exhibits a disk-like structure with a bluish hue, suggesting the presence of ongoing star formation within. Some degree of asymmetry or distortion seems present in the disk, possibly indicative of past interactions or internal processes. The overall color suggests a mix of older stellar populations in the central bulge and younger, bluer stars in the disk. There are a couple of prominent, bright features in the galaxy that could possibly be the light from HII regions. The galaxy's light appears to be relatively compact and faint compared to the other objects in the field.
