The galaxy presents as a spiral with a prominent, moderately sized bulge. The disk appears inclined, but not entirely edge-on, allowing for clear observation of spiral structure. Two distinct spiral arms are observed, though their winding is moderately tight. Evidence suggests that the bulge dominates the inner region with a tapering light profile towards the edge. The galaxy appears to be relatively isolated, with no clear indications of ongoing major merging activity. There may be some low-level disturbances within the disk, though the overall structure remains largely undisturbed. Faint reddish patches can be observed along the arms, suggestive of star forming regions.
