The galaxy presents a distinct spiral morphology, with prominent spiral arms emanating from a central bulge. The arms appear somewhat flocculent and exhibit a relatively open winding. The central bulge contributes significantly to the overall luminosity of the galaxy, with some indication of a moderate size relative to the disk. There is no obvious bar structure bisecting the bulge. The overall color suggests a diverse stellar population, with some bluer regions apparent within the spiral arms indicating ongoing star formation, as well as regions with a redder hue, suggesting the presence of older stellar populations. There are no obvious signs of a major merger or strong tidal disruption, but some subtle irregularities in the outer disk may indicate minor disturbances.
