The galaxy presents a generally smooth, elliptical morphology with a high degree of central concentration. The core region exhibits a bright, diffuse glow, fading gradually outward. The galaxy's overall shape appears somewhat flattened, approximating an oblate spheroid.  There may be a very subtle hint of a disk-like structure viewed edge-on, or perhaps a minor tidal disturbance, though the image resolution limits definitive assessment. The color profile suggests a population of older stars, with a general yellow/white hue dominating the light. Star formation appears to be low, as evidenced by the lack of strong blue light or distinct star-forming regions. There's no clear evidence of a major ongoing merger, though a slight asymmetry could indicate a minor interaction in the past.
