The galaxy presents a predominantly smooth morphology, with a high degree of central concentration. Its overall shape is more rounded than elongated, though not perfectly spherical. There are no obvious spiral arm structures or a well-defined disk component visible. There is a suggestion of minor disturbances, though the general structure does not appear to be undergoing a major merger. The central region exhibits a warmer, more yellow-orange hue, potentially indicating an older stellar population or dust obscuration. The outer regions show bluer colors, possibly suggesting a modest degree of ongoing star formation. The galaxy's physical size seems moderate, neither exceptionally large nor particularly compact relative to other galaxies at similar distances.