The galaxy appears to be a relatively smooth, elliptical or lenticular system. It exhibits a centrally concentrated bulge, with a gradual decrease in luminosity outwards from the core. There's a slight elongation of the galaxy shape, deviating minimally from a perfectly circular form. The color profile reveals a yellowish-white core, surrounded by a bluish halo. No prominent spiral arms, dust lanes, or distinct features indicative of recent major merger events are discernible. There is potential evidence of minor disturbances to the galaxy's morphology.
