The galaxy presents as a luminous, elliptical structure, with a concentrated bright central bulge that smoothly transitions into a more diffuse halo. There appears to be little to no resolved structure, such as spiral arms or distinct star-forming regions. The light distribution suggests a relatively smooth and homogenous stellar population. The galaxy's overall shape indicates a slight elongation, leaning towards a cigar shape. The color profile seems mostly uniform across the galaxy. There is no clear evidence of ongoing major mergers or tidal disturbances, the overall appearance implies relative dynamical stability.