The galaxy appears to be elliptical, with a smooth, concentrated light profile. The core is bright and yellowish-orange, indicative of an older stellar population. Moving outward from the core, the color transitions to a slightly bluer hue, suggesting the presence of some younger stars or a small amount of ongoing star formation in the outer regions. The galaxy's shape is somewhat elongated but not extremely so. There is no obvious evidence of spiral arms, prominent dust lanes, or major disturbances in its morphology. The overall impression is that of a relatively evolved system.
