The galaxy presents as a relatively smooth, elongated structure, appearing somewhat cigar-shaped. Its color profile suggests an older stellar population, with a dominant yellowish-orange hue concentrated toward the central region, likely the bulge. There is a subtle color gradient toward the outer edges of the disk, becoming slightly bluer. No distinct spiral arm features are visible. There is a faint, extended halo surrounding the main body of the galaxy. There does not appear to be any evidence of a major ongoing merger or significant tidal disturbances. The galaxy exhibits a red shift, indicating a relatively substantial distance from the observer.
