The galaxy presents as a centrally concentrated, elliptical or spheroidal system. It exhibits a smooth, relatively featureless morphology with a high degree of central light concentration. The light distribution suggests a dominant, well-established stellar population. The galaxy's overall shape appears close to circular, lacking a clearly defined disk component or significant tidal disturbances. There is an apparent absence of distinct spiral arms or prominent dust lanes, indicating a lack of significant ongoing star formation. The color profile implies a population dominated by older, redder stars, potentially indicative of an evolved stellar population. A hint of a faint, diffuse halo surrounds the brighter core. No signs of active galactic nuclei or significant merging activity are immediately apparent.
