The galaxy presents as a singular, centrally concentrated object with an approximately circular morphology. The light profile appears smooth and diffuse, lacking distinct spiral arm structures or a prominent bar. A central bulge region exhibits a higher luminosity, gradually fading into the outer regions. The galaxy displays a relatively uniform color gradient, appearing slightly more yellow-hued in the core and shifting towards a less saturated color in the outer regions, suggestive of an older stellar population. There is no obvious presence of tidal tails or other indications of recent major merger events, though minor disturbances can't be ruled out. The overall visual impression is consistent with an elliptical or lenticular galaxy type.
