This galaxy exhibits a distinct, elongated morphology, suggestive of a cigar shape when viewed from our perspective. The light distribution appears relatively smooth and concentrated toward the center. There is evidence of a subtle color gradient, shifting from a more yellow or orange hue in the central region to a slightly bluer tint at the outer edges. The overall structure does not indicate any major disturbances or ongoing merger events. The smooth light profile suggests a lack of significant star formation activity throughout the disk, however there may be regions of star formation. 