The galaxy appears as a moderately bright, elliptical or lenticular-like object. Its central region exhibits a concentrated luminosity, gradually decreasing outward. The galaxy's light profile is generally smooth, without apparent spiral arms or distinct features typically associated with disk galaxies. There is a subtle elongation in its morphology, suggesting it is not perfectly spherical, with an axis ratio greater than one. The primary color is a warm, yellow-orange hue, indicating a stellar population dominated by older, redder stars. There's no indication of recent or ongoing major star formation events, as the light is not dominated by blue colors associated with young, massive stars. Subtle asymmetry or minor disturbances cannot be ruled out, though the overall impression is of a well-established, relatively undisturbed system.
