The galaxy presents as a slightly elongated, disk-like structure, viewed at an oblique angle. The central region is bright and appears relatively smooth, exhibiting a yellowish hue that suggests a population of older stars. Surrounding the central region, a fainter, bluer disk is observed. This disk appears less uniform, with subtle variations in intensity that may indicate the presence of spiral arm structures or regions of active star formation. There is no obvious dust lane. The overall morphology suggests a relatively evolved galaxy, with signs of ongoing star formation in the outer regions of the disk. No major signs of interactions or significant disturbances are visible.
