The galaxy appears as a relatively compact object, roughly elliptical in shape. Its morphology is largely smooth, showing minimal signs of significant disturbances or distinct features like spiral arms or a prominent disk structure. The light profile suggests a high degree of central concentration with a gradual falloff in intensity outwards, suggesting a evolved system. There is a slight elongation visible. The galaxy exhibits a bluer color toward its central region with yellow/redder components. This may indicate a population of younger, hotter stars in the center, with older populations located in the outer regions. There are no indications of major mergers or tidal interactions.