The galaxy presents a generally smooth morphology. It exhibits an elongated shape, appearing cigar-shaped. There is some indication of a possible minor disturbance within the galaxy's structure, with regions of slightly irregular light distribution. A significant portion of the galaxy appears smooth, with a concentrated central region. Color gradients suggest variations in stellar populations, with a possible presence of ongoing star formation in some regions, as indicated by bluer hues. It may be undergoing a merger.
