The galaxy presents as a relatively face-on spiral, though with significant morphological disturbance. It is centrally concentrated, exhibiting a bright nucleus. The galaxy displays a smooth profile suggestive of a substantial bulge component. Some faint disk features are visible extending away from the nucleus, but they appear disrupted. Color gradients across the galaxy are subtle. The central bulge exhibits a yellowish-white hue, indicative of an older stellar population. Fainter bluish regions are observed in the outer disk, potentially suggestive of ongoing star formation, but are not very pronounced. Overall, the galaxy exhibits signs of recent or ongoing interaction, leading to its disturbed morphology, potentially involving a minor merger or tidal interaction, and some features that resemble tidal tails.
