The galaxy presents as a relatively smooth, disk-shaped structure with a prominent central bulge. The overall color suggests a population of older stars, giving it a yellowish hue, particularly concentrated in the central region. There's a hint of bluer color on one side suggesting a population of young stars. This galaxy likely shows signs of star formation, though it is minimal. There are no obvious spiral arm structures or dust lanes visible in this image. Based on the observed morphology, this galaxy appears to be an intermediate spiral type, leaning more towards a lenticular shape due to its smoothness. There is some subtle disruption visible indicating that it may be undergoing a minor interaction with a neighboring galaxy.
