The galaxy presents as a primarily smooth, elliptical morphology. The central bulge appears bright and concentrated, exhibiting a yellowish-white color indicative of an older stellar population. Moving outwards from the core, the luminosity gradually decreases, with a halo that appears more diffuse and slightly redder in hue. The galaxy appears as an oblate spheroid, leaning more towards a rounded shape than cigar-shaped. There is no visible evidence of strong spiral arms or a prominent disk structure. The overall structure appears undisturbed; no major signs of tidal disruption or ongoing merger events are apparent, although some minor irregularity cannot be ruled out with this resolution. Based on color and light profile, the system appears to be a relatively massive early-type galaxy with a low star formation rate.
