The galaxy appears as a single, relatively smooth and concentrated object. Its light profile is mostly uniform with a radial intensity gradient, appearing brightest at its core and gradually fading outwards. The shape is approximately elliptical, showing only a slight deviation from perfect roundness. There is no evidence of distinct spiral arms or a bar structure. The galaxy's color exhibits a yellowish or golden hue, which suggests a dominant population of older stars. There are no readily visible features of ongoing active star formation such as bright blue regions or irregular structures. There are no visible signs of significant tidal disturbances or close companion galaxies, indicating that this galaxy is likely not undergoing a major merging event.
