The galaxy presents an elongated, somewhat cigar-shaped morphology. A central bulge is discernable, exhibiting a yellowish hue, suggesting a population of older stars. Fainter, bluer light extends from the central region, potentially indicating ongoing star formation in a flattened disk. The galaxy's overall structure appears relatively smooth with some indication of minor disturbances in the disk. These disturbances could be tidal features caused by past interactions. The object is likely a disk galaxy seen at an inclined angle.
