The galaxy appears as an elongated, cigar-shaped structure. It exhibits a smooth, featureless morphology indicative of an early-type system. The color gradient transitions from a bluer hue in the upper regions to a yellower, possibly redder, hue in the lower section of the observed body, suggesting a gradient in stellar population ages or dust content. The light distribution is concentrated towards the center, which could signify a prominent central bulge. There may be a companion galaxy in the upper section of the image. Some signs of minor disturbance may be present as hinted at by the morphological properties.