The galaxy presents as a centrally concentrated object with a notable radial gradient in surface brightness. The core region exhibits a bright, yellowish-white hue, suggesting an older stellar population with less ongoing star formation. Moving outward from the core, the color transitions toward a bluer shade with hints of red, possibly indicative of younger stars or dust lanes, though the resolution makes definite features unclear. The overall morphology appears generally smooth and elliptical, with a slight elongation. No prominent spiral arms or other distinct morphological structures are discernible. The galaxy displays a moderate angular size. There's no evidence of a major ongoing merger or significant tidal disturbances. Based on the colors and morphology, this galaxy appears to be a relatively massive system with a moderate rate of star formation.
