The galaxy presents as a relatively smooth, elliptical morphology. It appears moderately inclined from our line of sight, displaying a somewhat elongated shape. A central bulge is discernible, exhibiting a brighter, more concentrated luminosity. The color profile suggests a population of older stars, likely a mix of yellow and red. The overall structure appears largely undisturbed, without obvious signs of active mergers or tidal distortions. Star formation appears to be relatively quiescent within the galaxy, based on the homogeneity of color and lack of intense blue regions indicative of recent starbursts. There is some evidence of a slight color gradient with a subtle bluer periphery compared to the core.