The galaxy presents as a centrally concentrated object, exhibiting a smooth, elliptical morphology. There is a clear radial gradient in surface brightness, with the core region being significantly brighter and transitioning smoothly to fainter outer regions. The galaxy appears nearly spheroidal, with no obvious disk or spiral arm structures. A slight elongation is observed, moving this galaxy to a slightly "in between" roundness. The color profile suggests the presence of a relatively old stellar population, with redder hues dominating the core and a subtle blueing trend towards the outer regions. No signs of active galactic nuclei are visible based on the central point source, which appears to have a smooth distribution of light. There is no apparent tidal debris or interaction features, indicating a relatively isolated evolutionary path.
