The galaxy presents a generally smooth appearance, suggesting it is relatively evolved. The dominant morphological feature is its elongated, cigar-like shape. The central region exhibits a concentrated brightness, indicating a possible galactic bulge or a higher density of stars. Moving outwards from the center, the light gradually fades, transitioning into fainter, diffuse regions on either end. There is a subtle color gradient, with the central bulge appearing more yellowish, possibly indicating an older stellar population, while the outer regions show hints of bluer tones. The bluer color suggests the presence of younger, hotter stars and regions of ongoing star formation. There are no obvious signs of spiral arm structures or a prominent disk, but some asymmetry is present, which could be caused by either recent interactions or internal dynamics. The object does not show any strong indications of ongoing major merger events.
