The galaxy presents a generally smooth, elliptical morphology. A central, luminous bulge dominates the structure, with a relatively diffuse and ill-defined outer halo. There is very little evidence of spiral arms or a prominent disk structure. The color gradient suggests a population of older stars with a primarily redder hue. We observe a moderate level of star formation with regions of bluer light scattered throughout. There is no obvious evidence of any major ongoing merger activity or significant tidal disturbances. There are no clear indications of dust lanes or obscuring material.
