The galaxy presents as a somewhat elongated object, indicative of a disk-like structure viewed at a high inclination. It possesses a centrally concentrated luminosity profile, suggesting a bulge component. The galaxy exhibits a relatively smooth texture with a lack of obvious spiral arm structure or significant dust lanes visible in this image. The color profile shows a somewhat bluer hue along the edges of the disk and a yellower color toward the center. This color variation might indicate ongoing star formation in the disk and a generally older stellar population in the central bulge. There is no sign of a recent major merger. The overall morphology suggests a relatively evolved spiral galaxy, possibly an early-type spiral or lenticular galaxy.
