The galaxy presents as a relatively smooth, elongated structure. It exhibits a prominent central bulge that appears yellowish in color, suggesting an older stellar population. The disk surrounding the bulge is bluer, hinting at the presence of younger, hotter stars and ongoing star formation, though the smoothness implies that the star formation is not intense. The galaxy's shape is notably cigar-like, appearing elongated rather than circular. There is no evidence of significant merger activity or major disturbances in its morphology. A faint and small amount of asymmetry is present in the disk, which could indicate a past minor interaction. Overall, the galaxy seems to be a relatively evolved system with a mix of old and younger stellar populations and is experiencing a low level of star formation.
