The galaxy presents an overall elongated, cigar-like shape. The central region displays a smooth, featureless appearance, lacking prominent spiral arms or a distinct nucleus. The light distribution across the galaxy is not uniform, exhibiting subtle variations in intensity and color. There may be a hint of a disk-like structure, but it is not well-defined. The color profile suggests a population of older stars, with a reddish hue dominating the central regions. However, there are also localized areas that appear bluer, indicating the presence of younger, hotter stars and possible ongoing star formation activity. There appears to be no significant signs of a recent or ongoing merger event. 
