The galaxy presents as a spiral, exhibiting a clear disk structure with visible spiral arms. These arms are somewhat loosely wound and appear to bifurcate, creating a complex pattern of star formation regions. The central bulge is moderately sized and displays a yellowish-orange hue, suggesting a population of older stars. The spiral arms, in contrast, show bluer regions indicative of ongoing star formation. There is evidence of a possible weak bar structure extending through the central region. Faint tidal features may be present, suggesting a past or ongoing interaction with a smaller galaxy. The galaxy has a general smooth texture, however there are hints of some irregular shapes, with two less prominent star clusters seemingly in the background, possibly indicating a minor ongoing merger.
