The galaxy presents as a somewhat elliptical, though not perfectly circular, object. A bright, concentrated central bulge dominates the structure, displaying a yellowish hue indicative of an older stellar population. The outer regions exhibit a smoother, less defined structure with a bluer color, hinting at ongoing, albeit relatively low, levels of star formation. There's a subtle indication of a possible disk structure, but the lack of defined spiral arms or distinct features suggests it's a relatively smooth and possibly evolved system. There is also a possibility the smooth nature of the disc could be due to it being obscured by dust. Overall, the galaxy appears to be a massive system. Evidence suggests there may be some merging activity present.
