This galaxy presents as an elliptical-like structure, exhibiting a smooth, diffuse morphology without prominent spiral arms or a well-defined disk. The central region appears brighter and more concentrated, with a slight color variation suggesting a relatively older stellar population residing in the core. The isophotes are somewhat elongated, transitioning from a round core into a cigar shaped halo. Faint blue tinges are visible at the edges of the galaxy, potentially indicating regions of younger star formation or a population of hotter, bluer stars in these outer regions. There are no readily apparent signs of major disturbances or ongoing mergers, although subtle asymmetries cannot be ruled out entirely. The overall appearance indicates that the galaxy is somewhere between an elliptical and lenticular galaxy.
