The galaxy presents a generally smooth, elliptical morphology. The light is concentrated towards the center, indicating a prominent bulge. The light fades towards the edges. There appears to be some hint of a disk, although it is subtle, and the galaxy is viewed at a slight angle. There is an absence of prominent spiral arm structures or significant dust lanes. The galaxy appears slightly elongated but close to round. The galaxy is yellowish-white, suggesting an older stellar population. There is no evidence of any major ongoing merger activity, though a subtle asymmetry could indicate a minor disturbance or previous interaction.
