The galaxy presents as a relatively face-on spiral with a moderately sized bulge. The spiral arms are loosely wound and extend outwards from the central bulge. A slight bar-like structure appears to be present. The overall color of the galaxy indicates a mix of stellar populations, with hints of blue indicating ongoing star formation, particularly within the spiral arms. The disk appears slightly inclined, resulting in an elliptical shape. There may be minor disturbances present, but no indication of a major merger. The spiral structure is well-defined. HI presence has also been detected within the galaxy.