The galaxy presents as a centrally concentrated system, appearing generally smooth in morphology. Its overall shape is elliptical, though not perfectly circular, displaying a slight elongation. A bright, prominent core dominates the central region, suggesting a high stellar density or possible active galactic nucleus. Moving outward from the core, the light gradually fades, indicating a decreasing stellar density. The color profile suggests a predominantly older stellar population, giving it a yellowish hue in the center. Fainter blue regions are visible in the surrounding arms, indicating the presence of some younger, hotter stars and active star formation, but it appears to be low in overall star formation rate. There may be minor evidence of slight disturbances, but it is generally undisturbed.
