The galaxy appears as a relatively smooth, elongated structure. The light distribution suggests a bulge-dominated morphology. The galaxy exhibits a color gradient, appearing bluish-white at the core, shifting to redder hues in the outer regions. This color variation could indicate differences in stellar populations or dust distribution. The overall shape is somewhat cigar-like, without any obvious spiral arms or distinct features. The galaxy shows some sign of disturbances, but appears to be mostly settled. This galaxy is of intermediate mass. The colors are consistent with ongoing star formation.
