This galaxy exhibits a relatively smooth, concentrated central region displaying a pronounced blue hue. Emanating from this central bulge, a fainter, elongated structure is observed, presenting a gradient shift towards redder wavelengths. Evident within this extended feature are subtle, irregular components indicative of either disrupted morphology or ongoing star formation. The overall form deviates from a perfectly circular profile, suggesting a departure from a simple elliptical type. Furthermore, there's a possible indication of tidal interactions or a minor merger event suggested by the irregular structure. The observed color gradient might reflect differing stellar populations, with bluer stars concentrated in the central region and older, redder stars prevalent in the extended structure. Further investigation is warranted to determine the exact nature of the morphological irregularities and the evolutionary history of the system.
