The galaxy presents as a flattened elliptical or lenticular form, with a notable central bulge exhibiting a yellowish hue, suggestive of an older stellar population. The galaxy's overall color appears reddish. The morphology indicates a system where star formation may be relatively subdued. The lack of defined spiral arms or prominent dust lanes suggests an evolved stellar system possibly approaching quiescence. There appears to be little evidence of recent major merging events, the galaxy seeming to be in a relatively relaxed state.
