The galaxy appears as a moderately elongated structure. A central, brighter region dominates the galaxy's overall form, suggesting a possible bulge or concentration of older stars. The color of this central region appears somewhat redder compared to other parts of the galaxy. Fainter extensions are visible, giving the galaxy a slightly irregular shape. These extensions exhibit a bluer hue, which could indicate regions of ongoing star formation. Evidence of possible interactions or minor disturbances exists, potentially influencing the observed morphology. Overall, the galaxy exhibits characteristics that suggest a complex formation history, with both older stellar populations and regions of more recent star formation activity contributing to its appearance.
