The galaxy presents an elliptical morphology, appearing generally smooth and rounded in form. A concentrated central bulge exhibits the brightest luminosity, diminishing gradually towards the outer regions of the galaxy. The color profile indicates a population of older stars, as evidenced by the reddish hues throughout the galaxy. While the galaxy appears largely undisturbed, subtle irregularities might suggest minor interactions or internal activity. There is no obvious spiral arm structure or prominent dust lane.
