The galaxy appears as a moderately luminous object, exhibiting a yellowish hue. The morphology suggests a relatively smooth, elliptical shape. There's a subtle elongation, deviating slightly from a perfect circular form. While the majority of the galaxy displays a consistent, featureless structure, there are faint indications of minor internal disturbances, possibly related to ongoing or past interactions. The central region is notably brighter, indicating a concentration of stellar density. The color profile suggests an older stellar population. Overall, the galaxy presents as a relatively evolved system with evidence of prior evolutionary processes.
