The galaxy appears as a somewhat diffuse, elliptical-like object, with a smooth profile. The light distribution is concentrated towards the center, with a gradual decrease in intensity towards the edges. The core of the galaxy appears a yellowish-orange color, indicative of an older stellar population with lower recent star formation. The galaxy does not show any prominent spiral arm structure or evidence of significant ongoing star formation. There is a faint, extended halo or envelope surrounding the main body of the galaxy. The shape of the galaxy is largely circular, with slight ellipticity. There are no obvious signs of a major ongoing merger, though subtle distortions may indicate minor interactions.