The galaxy presents as a well-defined, disk-shaped structure with a noticeable central bulge. The overall color profile indicates a higher concentration of older stellar populations, particularly within the bulge, which appears more yellow-red. The disk component shows some bluer regions but generally appears quite smooth with little evidence of strong spiral arm structures. The galaxy exhibits a moderate inclination relative to our line of sight, giving it an elliptical appearance. There are no obvious signs of recent major mergers or significant tidal disturbances in the immediate vicinity.
