The galaxy presents as a moderately luminous, elongated structure, likely a disk galaxy viewed at an oblique angle. The central bulge appears prominent and exhibits a yellowish hue, suggesting a population of older stars. The disk component displays a color gradient, transitioning from a yellowish-white center to a slightly bluer outer region. This color difference could indicate ongoing star formation within the galactic disk, particularly at its periphery. There is a lack of discernible spiral arm structure or distinct dust lanes; the galaxy appears relatively smooth overall, and there is not any sign of any recent or current merging events with other galaxies. The galaxy may be classified as an intermediate type.