The galaxy presents as a somewhat elliptical structure with a concentrated central bulge. The main body of the galaxy exhibits a generally smooth appearance, lacking prominent spiral arms or strong dust lane features. The color profile suggests a slightly higher concentration of older stellar populations, with a yellow-green hue at its center. The overall form indicates a likely transition from a spiral to an elliptical galaxy type, potentially a lenticular galaxy (S0). Minor disturbances or interactions are not immediately apparent in its overall structure, suggesting relative isolation or the late stages of any merging activity.
