The galaxy presents as a spiral type, exhibiting a disk-like structure seen at an oblique angle. Distinct spiral arms are observable, displaying a moderate winding pattern. The central bulge appears moderately sized, contributing significantly to the galaxy's overall luminosity. The spiral arms indicate ongoing star formation, evidenced by their slightly bluer coloration compared to the reddish hue of the central bulge. The galaxy appears isolated, without any immediately obvious major tidal features or signs of recent significant interactions with other galaxies. Evidence of a weak bar structure may be present in the central region.
