The galaxy presents a largely smooth and rounded morphology, exhibiting characteristics consistent with an elliptical galaxy classification. A concentrated central bulge, emitting a yellowish hue, dominates the galaxy's structure. The isophotes appear generally regular, lacking pronounced spiral arm features or irregular structures. There is faint blue light visible on the outer edges, with the object being relatively compact. There is no indication of any major ongoing merger events, although subtle asymmetries could point to minor tidal interactions. The central region exhibits higher luminosity, suggesting a higher stellar density compared to the outer regions. The galaxy appears to be a relatively evolved system, with a significant fraction of its stellar population likely comprised of older, redder stars.
