The galaxy presents as a relatively compact, elliptical morphology. The light distribution appears smooth and centrally concentrated, lacking prominent spiral arms or a well-defined disk structure. The galaxy exhibits a color gradient, appearing bluer towards the center, possibly indicating a higher concentration of younger, hotter stars in the core. There is some evidence of minor irregularities or disturbances in the outer regions, suggesting potential interactions or past mergers. The galaxy appears moderately luminous, implying a significant stellar population.
