The galaxy presents as a spiral, though some morphological disturbances are apparent. A substantial fraction of its light is concentrated in a moderately sized central bulge region, though it is not obviously dominant. Spiral arm structure appears present, although somewhat disrupted and not clearly defined. There are noticeable irregularities in the overall shape suggesting potential interactions or ongoing merger events. A faint disk is visible and oriented close to face-on with the line of sight. There appears to be at least weak bar structure.
