This galaxy exhibits a distinct, elongated morphology. The primary structure appears relatively smooth and undisturbed, with a high probability of not being a merger. The central region displays a notable concentration of light, suggesting a bulge component. The galaxy's overall color profile is dominated by redder wavelengths, potentially indicating an older stellar population and lower ongoing star formation rate. There is evidence of a slight gradient in color, with bluer hues visible towards the outer regions, possibly reflecting the presence of younger, hotter stars in a disk-like structure. The galaxy displays a high ellipticity, with a cigar-shaped appearance, suggestive of an edge-on disk galaxy or a prolate spheroidal galaxy. The projected size appears moderately compact. Overall, the galaxy appears to be a relatively evolved system with a significant bulge and hints of a disk component.
