The galaxy presents as a spiral type, with a dominant presence of well-defined spiral arms extending from a central bulge. The arms exhibit a patchy structure, suggestive of active star formation regions within the disk. The central bulge appears relatively small, and less prominent compared to the disk. The overall color of the galaxy is skewed towards bluer hues, particularly within the spiral arms, indicating the presence of a younger stellar population. The galaxy is not perfectly symmetrical, there is some minor disturbance that suggests a possible interaction or minor merger event. The disk appears relatively thin when viewed at an angle, as the galaxy appears to be a face-on view. Evidence of a bar structure is subtle but potentially present. Overall, the galaxy's morphology points towards a actively star-forming system with spiral arm structures.