The galaxy presents a distinct spiral morphology, with well-defined arms emanating from a central bulge. The spiral arms exhibit a flocculent structure, displaying a patchy distribution of star-forming regions. These regions are visibly bluer in color, indicative of the presence of younger, hotter stars. The winding of the arms appears relatively tight. A subtle bar structure can be inferred from the slight elongation of the bulge. The bulge itself is moderately sized, and appears somewhat luminous. The disk of the galaxy is inclined at a slight angle to our line of sight. The overall color of the galaxy is relatively blue, suggesting ongoing star formation. The lack of significant distortion in the galaxy's structure implies that it is likely not undergoing a major merger event.
