The galaxy presents a generally smooth morphology with a dominant central bulge.  The light distribution is concentrated towards the core, exhibiting a yellowish-orange hue, suggestive of an older stellar population.  There is a faint, diffuse disk component, but it is relatively unstructured and lacks prominent spiral arms. The galaxy is more elongated than spherical.  There is no clear indication of ongoing major merger activity, although some slight asymmetry could indicate minor gravitational interaction. Star formation appears to be occurring at a slow rate within the galaxy.
