The galaxy appears to be a fairly luminous object at a redshift of z~0.188. Its morphology suggests a mixed classification. A central, bright yellowish bulge dominates the galaxy's structure, implying an older stellar population in the core. There is evidence of a disk-like structure, though it is not a well-defined spiral. Instead, it appears somewhat amorphous and clumpy. The color gradients suggest ongoing, but not vigorous, star formation within the disk, characterized by subtle blueish-green regions. There seems to be some dust obscuration, particularly on one side of the galaxy, giving it a slightly uneven appearance. Overall, the galaxy exhibits characteristics of both spiral and elliptical galaxies, and shows no strong signatures of an ongoing major merger. There may be some slight disturbance of its overall shape.
