The galaxy presents as an elongated, cigar-shaped structure. It has a smooth, diffuse appearance with no prominent spiral arms or distinct features visible. The light is concentrated towards the center, suggesting a bulge-like morphology. There's a color gradient present, transitioning from a central reddish-orange hue to bluer edges, indicative of differing stellar populations or dust distribution within the galaxy. The lack of defined structures suggests a relatively evolved galaxy, possibly an elliptical or lenticular type with ongoing, moderate star formation. There is little evidence of a major ongoing merger, though a minor interaction cannot be ruled out due to the slight irregularities at the galaxy's periphery.
