This galaxy presents as a spiral type, viewed at an oblique angle. It exhibits a prominent central bulge, surrounded by a relatively well-defined disk. Indications of spiral arm structure are visible within the disk, estimated to have two main arms. The winding of these arms appears to be intermediate. The colour distribution shows a yellowish hue concentrated in the central bulge region, while the outer disk appears bluer, suggesting the presence of younger stellar populations. There may be a bar-like structure present that extends across the central region of the galaxy, though this is not very clear. No signs of major ongoing mergers or significant tidal disturbances are obviously visible in this image.
