The galaxy presents a generally smooth appearance, with a slightly elongated, cigar-like shape. It appears as a flattened ellipsoid. The central region exhibits a higher concentration of light with a yellowish hue, suggesting an older stellar population or a significant dust presence. Moving outwards from the center, the light becomes less concentrated and shifts towards a bluer color, which may indicate the presence of younger, hotter stars. There are no clearly discernible spiral arms or prominent features, and there is no obvious indication of a major merger event, though some minor distortions are subtle. Overall, it is a relatively well-defined, smooth galaxy.
