This galaxy presents as a spiral-type morphology, likely viewed at an oblique angle to our line of sight. The central bulge appears moderately sized and displays a yellowish hue, which may indicate an older stellar population. Two prominent spiral arms are clearly visible, exhibiting a relatively open winding pattern. There is some indication of a bar structure within the central region of the galaxy. Star formation appears to be distributed throughout the disk, particularly within the spiral arms. No major signs of strong gravitational disturbance or ongoing merger events are immediately apparent, though some minor asymmetries may be present within the arm structures. The galaxy is not particularly inclined, with a ratio of major to minor axes that is closer to one.
