The galaxy presents as a relatively smooth, elliptical morphology. The central region exhibits a concentrated, bright core that appears yellowish-white in color. Moving outward from the core, the light gradually fades into a more diffuse, reddish-hued halo. The overall shape deviates slightly from perfectly circular, tending toward a mild elongation. There is no apparent evidence of spiral arms or significant dust lanes visible in this imagery. A faint hint of blue on the outer edges suggests the potential for some limited, ongoing star formation. No signs of significant tidal disturbances or ongoing merger activity are immediately apparent. The galaxy appears as a fairly undisturbed system, with a light profile consistent with an evolved stellar population.
