The galaxy presents a smooth, elliptical morphology with a high degree of roundness. It appears largely featureless, lacking prominent spiral arms or a distinct central bar. The light distribution suggests a centrally concentrated luminosity profile, gradually decreasing towards the outer edges. The galaxy exhibits a color gradient, with the core appearing more yellow/orange and transitioning to a slightly redder hue at the periphery. There is no evidence of ongoing major merging events or significant tidal disturbances. The galaxy is likely composed of a relatively older stellar population. There is a hint of a faint, diffuse halo surrounding the main body. Star formation rate is estimated to be relatively low.