The galaxy presents as an elongated structure, indicative of a possible elliptical morphology, though a highly inclined disk cannot be ruled out. The central region exhibits a concentration of light, suggesting a prominent bulge or core. The color profile across the galaxy varies, with a yellowish hue dominating the core region, potentially indicating an older stellar population. Fainter, bluer extensions are visible along the major axis, suggesting the presence of younger stars or regions of active star formation, though limited in scale. There appears to be a subtle asymmetry in the outer regions. The overall texture appears smooth, although at this resolution, finer details of internal structure are not readily discernible.
