The galaxy presents an overall elliptical morphology, with a smooth light distribution, appearing largely featureless. A bright central bulge dominates the galaxy's luminosity. The color gradient suggests an older stellar population within the bulge.

A fainter, diffuse disk component surrounds the central bulge. There are no obvious spiral arms or distinct dust lanes visible. The galaxy's overall color suggests a galaxy transitioning between active star formation and quiescence. The absence of strong blue color suggests relatively low ongoing star formation. There does appear to be some minor disturbance or asymmetry in the outer regions, which could be evidence of a past or ongoing minor merger event.
