The galaxy appears to be a relatively small, well-defined system, exhibiting a flattened, disk-like structure. Its color profile suggests an intermediate stellar population with a notable central concentration of older, yellow stars, grading into a bluer population in the outer regions of the disk. A slight asymmetry is visible, possibly indicative of a minor interaction or internal disturbance. There are no obvious spiral arm features in the image, suggesting it may be a lenticular galaxy.
