The galaxy presents a generally smooth morphology, with a high degree of central concentration. Its overall shape appears somewhat elliptical, exhibiting a transition between round and elliptical, without a highly elongated or cigar-like form. There is a bright central bulge, which dominates the galaxy's luminosity profile. A diffuse, extended halo surrounds the central region, gradually fading into the background. Faint blue tones are visible in the outer regions of the galaxy, potentially indicating regions of recent or ongoing star formation, though these are not particularly pronounced. There is no obvious indication of major disturbances or mergers, with a seemingly relaxed structure. Given the color profile, it would be expected that the stellar mass is quite high.
