The galaxy presents as an elongated, cigar-shaped structure with a relatively smooth overall appearance. Its central region exhibits a concentrated luminosity, suggesting a dense stellar population or active galactic nucleus. Moving outward from the center, the brightness diminishes, with the disk appearing somewhat thin. Faint hints of bluer regions are visible along the edges of the disk, possibly indicating areas of ongoing star formation. There may be a slight indication of minor disturbances within the galactic structure. Based on the color profile, the dominant stellar population likely consists of older, redder stars, with younger, bluer stars present in a smaller proportion.
