The galaxy presents as a somewhat diffuse, elliptical structure with a high degree of central concentration. Its morphology appears largely smooth, lacking prominent spiral arms or a well-defined disk. The light distribution suggests an older stellar population. There's a slight indication of tidal disturbance or a minor interaction, potentially evidenced by faint asymmetrical light distribution. The red color of the image suggests a low rate of star formation and dominance of older stars. The shape of the galaxy is somewhere between round and elliptical, but closer to elliptical. There may be a companion galaxy to the side causing these disturbances.