The galaxy presents as a slightly inclined spiral, exhibiting a relatively high degree of symmetry. A prominent central bulge dominates the overall light distribution. Faint spiral arm structures are observed extending from the central region. The arms are tightly wound, possessing fragmented star forming regions within the disk. Patches of blue emission hint at recent star formation. The disk appears relatively thin. There is no evident central bar feature. The outer regions of the galaxy exhibit a smoother distribution of light, transitioning into the background sky. There is no evidence of a major merger or tidal disturbance in this image. The galaxy has an elliptical appearance.
