The galaxy presents as a largely smooth, elliptical morphology with a pronounced central bulge. The light distribution appears highly concentrated, with a radial gradient decreasing in intensity from the core outwards. The color profile suggests a dominant population of older stars, exhibiting redder hues, particularly in the innermost regions. There is no discernible spiral arm structure or significant dust lane obscuration, consistent with a lack of ongoing, large-scale star formation. Overall, the galaxy exhibits a morphology indicative of an early-type system, likely an elliptical or lenticular galaxy.
