The galaxy presents as a relatively smooth object, with a dominant central bulge. The bulge exhibits a yellowish-white hue, suggesting a population of older stars. A faint, slightly bluer disk component appears to surround the central bulge, though the structure is largely featureless. There are no prominent spiral arms or dust lanes visible. The galaxy displays a generally elliptical shape, though it is fairly round, suggesting it is not viewed edge-on. There is no clear evidence of any ongoing major merger activity, though slight asymmetry in the outer regions suggests a minor interaction or disturbance may have occurred in the past. Overall, the galaxy appears to be a passively evolving system with a dominant older stellar population.
