This galaxy appears to be a relatively smooth, centrally concentrated system. The morphology suggests a dominant spheroidal component, with a high degree of circular symmetry. There is a noticeable color gradient, with the central region exhibiting a yellowish hue that transitions to a redder color in the outer regions. This color gradient could indicate an older stellar population in the galaxy's core, with relatively low levels of ongoing star formation in the galaxy as a whole. Faint tidal features are visible near the galaxy, although they are very slight. There is no obvious disk structure, or spiral arms. The galaxy's overall appearance suggests that it is a massive system.
