The galaxy appears as a centrally concentrated, relatively smooth object. The light distribution suggests a spheroidal morphology, potentially an elliptical galaxy or a lenticular galaxy viewed at a shallow inclination. There is a discernible radial fall-off in luminosity from the core outwards. The central region exhibits a bright, concentrated core that fades into a less luminous halo or extended envelope.

There is subtle elongation in the morphology, giving it a slightly oval appearance. No distinct spiral arms or well-defined disk-like structures are apparent. There is no obvious major tidal disturbance or signs of a recent major merger event. A subtle, minor asymmetry is visible in the outer regions, hinting at a possible minor interaction or accretion event in its past. The color profile suggests a population of older stars, with a redder color dominating the overall light.
