The galaxy presents a largely smooth, elliptical morphology. The central region exhibits a high concentration of light, suggesting a dense stellar population, which gradually diffuses outwards. The overall color profile indicates the presence of older stars. The lack of distinct spiral arms or prominent dust lanes is consistent with an elliptical classification. A subtle elongation is observed, deviating slightly from a perfectly circular form. There is no strong evidence of active galactic nuclei activity or significant ongoing star formation based on the color profile. There are some minor disturbances visible within the outer regions, suggesting either a possible minor merger or tidal interactions.
