The galaxy presents an elongated, somewhat disturbed morphology. It appears to exhibit a bulge, although it is not clearly defined. The light distribution suggests a central concentration of older stars and possibly dust extinction. There is indication of a disk component, but it is not fully resolved. The color profile shows gradients, with the central regions appearing redder than the outer areas, which are bluer, suggesting recent star formation. There are areas with clumpy formations. These may be star-forming regions within the galaxy. Overall, there may be evidence of recent or ongoing minor disturbances.
