The galaxy presents as a relatively compact, luminous object. It exhibits a smooth, elliptical morphology with a high degree of roundness and a concentrated central region. There is a subtle color gradient visible, with the core appearing somewhat yellower than the outer regions. This suggests a higher concentration of older stellar populations in the galactic nucleus. No distinct spiral arms or prominent dust lanes are observed, indicating a lack of significant ongoing star formation or a well-mixed stellar population. There is no obvious evidence of a major merger event. Minor disturbances cannot be ruled out, based on the apparent smoothness of the galaxy's profile.
