The galaxy presents a complex morphology, appearing to be in a potential merger state. A dominant, relatively smooth and rounded component is observed, exhibiting a yellowish-white hue, suggesting a population of older stars. Extending from this central region is a fainter, bluish, plume-like feature, which might be indicative of tidal debris or disturbed spiral arm structure resulting from gravitational interaction with another galaxy. There's a slight asymmetry to the overall form, with the extension skewed toward one side. The color gradient from the core outwards suggests ongoing, albeit possibly low-level, star formation activity. The central region appears somewhat condensed, suggesting a relatively high density of stars in that region.
