The galaxy presents a primarily disk-like morphology, with the disk oriented at an inclined angle relative to our line of sight. A prominent central bulge is apparent, exhibiting a concentrated luminosity profile with a yellowish hue, indicating a substantial population of older stars. Faint spiral arms are visible extending outward from the central bulge, but are only just discernible. The overall color of the galaxy suggests ongoing star formation, primarily within the disk component. The galaxy does not show any obvious signs of a major merger or significant tidal disturbances.
